HAL Id: hal-01377741
https://hal.inria.fr/hal-01377741
Submitted on 9 Nov 2016
HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.
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�
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 . m−1"
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 . m−1"
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 . m−1"
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 . m−1"
t = 17 d ay s
LR deterministic simulation (1282) Spectrum of
w|t=0 and B˙
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 . m−1"
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