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Stochastic subgrid tensor for geophysical flow modeling

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HAL Id: hal-01377741

https://hal.inria.fr/hal-01377741

Submitted on 9 Nov 2016

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Stochastic subgrid tensor for geophysical flow modeling

Valentin Resseguier, Etienne Mémin, Bertrand Chapron

To cite this version:

Valentin Resseguier, Etienne Mémin, Bertrand Chapron. Stochastic subgrid tensor for geophysical flow modeling. 8th European Postgraduate Fluid Dynamics Conference, Jul 2016, Varsovie, Poland.

�hal-01377741�

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STOCHASTIC SUBGRID TENSOR FOR GEOPHYSICAL MODELING

Valentin Resseguier, Etienne Mémin, Bertrand Chapron

Conservations

(mass, linear momentum, …)

Navier-Stokes

Boussinesq

SQG under Moderate Uncertainty

QG MU

Uncertainty

D Dt

Systematic derivation of random models with the

new

Usual SQG relationship and transport under uncertainty of buoyancy

Good illustration of our stochastic transport

Simulations done with homogeneous small-scale velocity Assumption:

Velocity decomposition: with

From stochastic calculus theory, we proofed:

QG assumption under strong uncertainty:

• kills the interior dynamics

• creates horizontal velocity divergence

• provides a diagnostic relation

Transport under location uncertainty

Conclusion

Quantification of the dynamics errors:

- Diagnostic for numerical simulations (mesh refinements, …)

- Ensemble data assimilation and forecasts

Rigorous identification of sudgrid dynamics effects

Taking into account likely small-scale dynamics (stochastic backscatter)

Forecast of likely distinct scenarios

Motivations

Advection

Inhomogeneous and anisotropic

diffusion

Balanced

energy exchanges

D⇥

Dt = @

t

⇥ + w

?

· r ⇥ + B ˙ · r ⇥ r ·

✓ 1

2 a r ⇥

= 0

Multiplicative random

forcing Drift

correction

v = w + B˙

8<

:

w B˙

large-scale velocity

uncorrelated in time, divergence-free, correlated in space, Gaussian,

inhomogeneous and anisotropic

y(m)

x(m)

t = 0 d ay s

0 2 4 6 8

x 105 0

5

10 x 105

−1

−0.5 0 0.5 x 101 −3

Initial condition

10−5 10−4

100 102 104

|ˆf(κ)|2

κ(rad.m−1) Initial spectrum ofwandσdBt

-5/3

x ( m)

y(m)

t = 17 d ay s

0 2 4 6 8

x 105 0

2 4 6 8

x 105

−1

−0.5 0 0.5 x 101 −3

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ!

r a d . m1"

t = 17 d ay s

Reference: HR deterministic simulation (5122)

One realization: better small-scale representation

x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m−1"

t= 17 d ay s

Ensemble of simulations

x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m−1"

t= 17 d ay s x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m−1"

t= 17 d ay s x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m−1"

t= 17 d ay s x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m−1"

t= 17 d ay s x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m−1"

t= 17 d ay s x ( m)

y(m)

t= 17 d ay s

0 2 4 6 8 10

x 105 0

2 4 6 8

x 105

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ! r a d . m1"

t= 17 d ay s

x ( m)

y(m)

t = 17 d ay s

0 2 4 6 8

x 105 0

2 4 6 8

x 105

−1

−0.5 0 0.5 x 101 −3

10−5 10−4

10−6 10−4 10−2

|ˆ b(κ)|2

κ!

r a d . m1"

t = 17 d ay s

LR stochastic simulation (1282)

x ( m)

y(m)

t = 17 d ay s

0 2 4 6 8

x 105 0

2 4 6 8

x 105

−1

−0.5 0 0.5 x 101 −3

10−5 10−4

10−6 10−4 10−2

|ˆb(κ)|2

κ!

r a d . m1"

t = 17 d ay s

LR deterministic simulation (1282) Spectrum of

w|t=0 and

x ( m)

y(m)

Me an e r r or

0 2 4 6 8

x 105 0

2 4 6 8 10x 105

0.5 1 1.5 2 x 10−4

x ( m)

y(m)

O u r e st i mat i on

0 2 4 6 8

x 105 0

2 4 6 8

x 105

0.5 1 1.5 2 x 10−4

x ( m)

y(m)

Ran d om I C

0 2 4 6 8

x 105 0

2 4 6 8

x 105

0.5 1 1.5 2 x 10−4

10−5 10−4

10−8 10−6 10−4

|ˆe(κ)|2

κ!

r a d . m1"

S p e c t r u m of t h e e r r or s an d i t s e st i mat i on at t = 13 d ay s

Our error Our estimation

Error with random IC Estimation random IC

Errors estimation

x ( m)

y(m)

S t an d ar d d e v i at i on

0 5 10

x 105 0

2 4 6 8

x 105

x ( m)

y(m)

S k e w n e ss

0 5 10

x 105 0

2 4 6 8

x 105

x ( m)

y(m)

l og( K u r t osi s-3)

0 5 10

x 105 0

2 4 6 8

x 105 x ( m)

y(m)

Me an at t = 17 d ay s

0 5 10

x 105 0

2 4 6 8

x 105

−2

−1 0 1 2

−4

−2 0 2

−1

−0.5 0 0.5 x 101 −3

0 0.5 1 x 101.5 −4

Point-wise moments:

variability, extreme events, … Description

Random transport applicable to any dynamics

Better representation of small scales

Extreme events

Good errors estimation in location and amplitude

Likely scenarios

code available online: link from Fluminance website - V. Resseguier

Description

r · u / r

?

· u

Geostrophic balance

Horizontal Diffusion

f ⇥ u = 1

b rp0 + a

2 u

Modified geostrophic balance

Testbed data:

very high-resolution model outputs

Gula, J., Molemaker, J., and McWilliams J.

"Gulf Stream dynamics along the southeastern US seaboard.”

Journal of Physical Oceanography 45.3 (2015): 690-715.

x(m)

y(m)

Te mp e r at u r e

4 5 6 7 8

x 105 0

1 2 3 4 5 6

x 105

15 20 25

x(m)

y(m)

Te mp e r at u r e

0 2 4 6 8

x 105 0

2 4 6 8 10

x 105

15 20 25

Original Filtered

Results

x(m)

y(m)

D i v e r ge n c e

4 6 8

x 105 0

2 4 6

x 105

−1 0 1 x 10−5

x(m)

y(m)

E st i mat i on

4 6 8

x 105 0

2 4 6

x 105

−2

−1 0 1 2

x 10−12

Conclusion

Frontolysis / frontogenesis on warm / cold side of fronts

Estimation of horizontal divergence or diffusive coefficient and subgrid variance

Strong uncertainty assumption verified
 a posteriori for the Gulf Stream


during wintertime at mesoscales

SQG under Strong Uncertainty

w = w 1

2r · a a = T

Références

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