How to treat the coupling issue of the Saint-Venant-Exner system of - - PowerPoint PPT Presentation

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How to treat the coupling issue of the Saint-Venant-Exner system of - - PowerPoint PPT Presentation

How to treat the coupling issue of the Saint-Venant-Exner system of equations Philippe Ung 1 , 4 joint work with Emmanuel Audusse 1 , 2 , Christophe Chalons 3 1 Team ANGE CEREMA, Inria Rocquencourt, LJLL 2 LAGA Universit e Paris XIII 3


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How to treat the coupling issue of the Saint-Venant-Exner system of equations

Philippe Ung1,4

joint work with Emmanuel Audusse1,2, Christophe Chalons3

1Team ANGE – CEREMA, Inria Rocquencourt, LJLL 2LAGA – Universit´

e Paris XIII

3LMV – Universit´

e de Versailles Saint-Quentin-en-Yvelines

4MAPMO – Universit´

e d’Orl´ eans

Egrin June 1st, 2015

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Context & Motivations Numerical scheme Test cases Discussion

Outline

Context & Motivations Numerical scheme Test cases Discussion

  • Ph. Ung

Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 2 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Context & Motivations

  • Ph. Ung

Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 3 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Motivations

Framework

Sediments transport is responsible of modification of river beds. 2 processes of sediments transport: by suspension: particles can be found on the whole vertical water depth and rarely be in contact with the bed, by bedload: particles are moving near the bed by saltation and rolling.

Figure: Processes of sediment transport.

Thereafter, we only focuse on the bedload transport.

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Saint-Venant–Exner equations

The model

In the literature, most of industrial codes use the Saint-Venant–Exner model.        ∂tH + ∂x (Q) = 0, (1a) ∂tQ + ∂x Q2 H + gH2 2

  • = −gH∂xB − τ

ρ. (1b) ∂tB + ∂xQs = 0, (1c) Coupled model between: the Saint-Venant equations (aka shallow-water equations): (1a)–(1b)

x z U(t, x) B(t, x) H(t, x)

H(t, x): water height, Q(t, x) = HU: discharge, B(t, x): bottom topography, with x ∈ Ω ⊆ R, t 0.

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Saint-Venant–Exner equations

The model

τ is defined by the Manning formula, τ = ρgH Q|Q| H2 K 2

s R4/3 h

, (2) where, in the particular case of a rectangular channel with width l, the hydraulic radius Rh reads Rh = lH l + 2H .

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Saint-Venant–Exner equations

The model

the Exner equation (1c) where Qs(t, x) is the solid transport flux defined by Qs =

  • g(ρs − ρ)d3

ρ Q⋆

s (τ ⋆; τ ⋆ c ) τ ⋆

|τ ⋆| (3) and the Meyer-Peter-M¨ uller formula, Q⋆

s = A (|τ ⋆| − τ ⋆ c )3/2 +

(4) with                A a constant, ρs, ρ

  • resp. the mass densities of the solid and fluid phases,

g the gravitational acceleration, τ ⋆ the shear stress (aka Shields parameter), τ ⋆

c

the critical value for the initiation of motion, d the grain diameter.

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Context & Motivations Numerical scheme Test cases Discussion

Saint-Venant–Exner equations

The model

A more practical expression of the solid discharge Grass formula, Qs = AgU |U|m−1 (5) where Ag is an empirically determined constant and 0 < m < 4.

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Context & Motivations Numerical scheme Test cases Discussion

Saint-Venant–Exner equations

The model

The Saint-Venant–Exner equations can be rewritten in a vectorial form, ∂t ˜ W + ∂xF( ˜ W ) = S( ˜ W ), (6) where ˜ W =   H HU B  , F( ˜ W ) =     HU HU2 + gH2 2 Qs    , S( ˜ W ) =   −gH∂xB  . Quasilinear form: ∂t ˜ W + A( ˜ W )∂x ˜ W = S( ˜ W ), where A is the jacobian matrix of F.

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Context & Motivations Numerical scheme Test cases Discussion

Motivations

Numerical aspect

Two strategies to approximate the solution of the system: splitting and non-splitting methods.

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Context & Motivations Numerical scheme Test cases Discussion

Motivations

Numerical aspect

Two strategies to approximate the solution of the system: splitting and non-splitting methods. The problem of choice between these two methods remains when considering “fast flow” (Hudson et al, 2003 & 2005):

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Motivations

Numerical aspect

Two strategies to approximate the solution of the system: splitting and non-splitting methods. The problem of choice between these two methods remains when considering “fast flow” (Hudson et al, 2003 & 2005): the splitting method injects numerical instabilities,

Figure: Free surface (top) and Bottom topography (bottom)

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Motivations

Numerical aspect

the non-splitting method allows to correct these instabilities,

  • Roe-type solver (Hudson et al. 2003 & 2005, Murillo and

Garcia-Navarro 2010),

  • Intermediate Field Capturing Riemann solver (Pares 2006,

Pares et al. 2011),

  • Relaxation scheme (Delis et al. 2008, ABCDGJSGS 2011),
  • Non Homogeneous Riemann solver (Benkhaldoun et al. 2009),
  • Godunov-type method based on a three-waves Approximate

Riemann Solver (ARS).

  • Ph. Ung

Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 11 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation

Properties & Main definitions

Positivity of water height, H 0 ,

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation

Properties & Main definitions

Positivity of water height, H 0 , Well-balanced property or ability to preserve steady states of the lake at rest, U = 0 , H + B = Cte .

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation

Properties & Main definitions

Positivity of water height, H 0 , Well-balanced property or ability to preserve steady states of the lake at rest, U = 0 , H + B = Cte . Froude number, Fr = |U| √gH . (7) Fr < 1 Fluvial regime, Fr = 1 Transcritical regime, Fr > 1 Torrential regime.

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Objective

Main objective

Developping a non-splitted method to solve the Saint-Venant–Exner system.

Strategy

Propose a Godunov-type method to solve the Saint-Venant–Exner equations based on the design of a three-wave Approximate Riemann Solver which is able to degenerate to an ARS satisfying all these properties together when the solid flux is null, sufficiently easy to compute.

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Discretization

Space discretization Ω, ∀i ∈ Z

x xi−1/2 xi+1/2 Ci ∆xi = xi+1/2 − xi−1/2 xi

Nx: Number of cells. Time discretization t 0, ∀n ∈ N tn+1 = tn + ∆tn , ∆t > 0. In the following, we denote ∆xi = ∆x , ∆tn = ∆t .

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Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 15 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Main ideas

Notations: ∀X ∈ {H, HU, B}, XL ≈ 1 ∆x

−∆x

X(x)dx ; XR ≈ 1 ∆x ∆x X(x)dx ; Xi ≈ 1 ∆x

  • Ci

X(x)dx .

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Main ideas

Notations: ∀X ∈ {H, HU, B}, XL ≈ 1 ∆x

−∆x

X(x)dx ; XR ≈ 1 ∆x ∆x X(x)dx ; Xi ≈ 1 ∆x

  • Ci

X(x)dx . At tn, ˜ W n

i = (W n i , Bn i ) = (Hn i , Hn i Un i , Bn i )T a given piecewise

constant approximate solution,

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Main ideas

Notations: ∀X ∈ {H, HU, B}, XL ≈ 1 ∆x

−∆x

X(x)dx ; XR ≈ 1 ∆x ∆x X(x)dx ; Xi ≈ 1 ∆x

  • Ci

X(x)dx . At tn, ˜ W n

i = (W n i , Bn i ) = (Hn i , Hn i Un i , Bn i )T a given piecewise

constant approximate solution, Building an approximate solution of the Riemann problem at each interface xi+1/2,

  • Ph. Ung

Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 16 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Main ideas

Notations: ∀X ∈ {H, HU, B}, XL ≈ 1 ∆x

−∆x

X(x)dx ; XR ≈ 1 ∆x ∆x X(x)dx ; Xi ≈ 1 ∆x

  • Ci

X(x)dx . At tn, ˜ W n

i = (W n i , Bn i ) = (Hn i , Hn i Un i , Bn i )T a given piecewise

constant approximate solution, Building an approximate solution of the Riemann problem at each interface xi+1/2, Definition of ˜ W n+1

i

= (W n+1

i

, Bn+1

i

) by calculating the average value of the juxtaposition of these solutions in each cell Ci at time tn+1.

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Riemann problem

A simple Approximate Riemann Solver composed by three waves propagating with velocities λL, λ0 = 0 and λR such as

λ0 λL λR x t (W ⋆

R, B⋆ R)

(W ⋆

L , B⋆ L)

(WR, BR) (WL, BL)

Figure: Local Riemann problem

λL 0 λR. gives an approximate Riemann solution associated with initial data (W (0, x), B(0, x)) = (WL, BL) , x < 0, (WR, BR) , x > 0. CFL condition: ∆t <

∆x 2 max(|λL|, λR).

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Consistency

Consistency F( ˜ WR)−F( ˜ WL)−S

  • ˜

WL, ˜ WR

  • = λL( ˜

W ∗

L − ˜

WL)+λR( ˜ WR − ˜ W ∗

R) ,

with lim

˜ WL, ˜ WR → ˜ W ∆x → 0

1 ∆x S

  • ˜

WL, ˜ WR

  • = (0, −gH∂xB, 0)T .

Relations of consistency in the integral form:

             HRUR − HLUL = λL (H⋆

L − HL) + λR (HR − H⋆ R) ,

(8)

  • HRU2

R + gH2 R

2

  • HLU2

L + gH2 L

2

  • + g∆x{H∂xB}

= λL (H⋆

LU⋆ L − HLUL) + λR (HRUR − H⋆ RU⋆ R) ,

(9) QsR − QsL = λL (B⋆

L − BL) + λR (BR − B⋆ R) .

(10)

  • Ph. Ung

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Numerical approximation of the Saint-Venant–Exner equations

Definition of the intermediate states

Relations of continuity across the stationary wave:

H⋆

L + B⋆ L = H⋆ R + B⋆ R,

(11) H⋆

LU⋆ L = H⋆ RU⋆ R.

(12) We add a minimization problem min F(B⋆

L, B⋆ R) =

  • ||BL − B⋆

L||2 + ||BR − B⋆ R||2

u.c. λL (B⋆

L − BL) + λR (BR − B⋆ R) − (QsR − QsL) = 0

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation of the Saint-Venant–Exner equations

Definition of the intermediate states

Relations of continuity across the stationary wave:

H⋆

L + B⋆ L = H⋆ R + B⋆ R,

(11) H⋆

LU⋆ L = H⋆ RU⋆ R.

(12) We add a minimization problem min F(B⋆

L, B⋆ R) =

  • ||BL − B⋆

L||2 + ||BR − B⋆ R||2

u.c. λL (B⋆

L − BL) + λR (BR − B⋆ R) − (QsR − QsL) = 0

B⋆

L = BL +

λL λ2

L + λ2 R

∆Qs, (13) B⋆

R = BR −

λR λ2

L + λ2 R

∆Qs, (14)

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Definition of the intermediate states: Well-balanced property

Q⋆ := H⋆

LU⋆ L = H⋆ RU⋆ R,

Q⋆ = QHLL − g λR − λL ∆x{H∂xB}, (15) with

QHLL = λRHRUR − λLHLUL λR − λL −

  • HRU2

R + gH2 R

2

  • HLU2

L + gH2 L

2

  • λR − λL

,

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Definition of the intermediate states: Well-balanced property

Q⋆ := H⋆

LU⋆ L = H⋆ RU⋆ R,

Q⋆ = QHLL − g λR − λL ∆x{H∂xB}, (15) with

QHLL = λRHRUR − λLHLUL λR − λL −

  • HRU2

R + gH2 R

2

  • HLU2

L + gH2 L

2

  • λR − λL

,

Well-balanced property ensures by {H∂xB} =      HL + HR 2∆x min (HL, ∆B) if ∆B⋆ 0, HL + HR 2∆x max (−HR, ∆B) if ∆B⋆ < 0.

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Numerical approximation of the Saint-Venant–Exner equations

Definition of the intermediate states: Positivity of the water height

H⋆

L = HHLL +

λR λR − λL ∆B⋆, (17) H⋆

R = HHLL +

λL λR − λL ∆B⋆, (18) with HHLL = λRHR − λLHL λR − λL − 1 λR − λL (HRUR − HLUL) . (19)

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation of the Saint-Venant–Exner equations

Definition of the intermediate states: Positivity of the water height

H⋆

L = HHLL +

λR λR − λL ∆B⋆, (17) H⋆

R = HHLL +

λL λR − λL ∆B⋆, (18) with HHLL = λRHR − λLHL λR − λL − 1 λR − λL (HRUR − HLUL) . (19) If ∆B⋆ 0, If ∆B⋆ < 0, λR ˜ H

⋆ R = max (λRH⋆ R, 0),

λL ˜ H

⋆ L = max (λLH⋆ L, 0)

λL ˜ H

⋆ L = λLH⋆ L − λR

  • H⋆

R − ˜

H

⋆ R

  • ,

λR ˜ H

⋆ R = λRH∗ R − λL

  • H⋆

L − ˜

H

⋆ L

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Numerical approximation of the Saint-Venant–Exner equations

Definition of the wave velocities

The main issue comes from the choice of λL and λR.

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Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 22 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation of the Saint-Venant–Exner equations

Definition of the wave velocities

The main issue comes from the choice of λL and λR. Recall A( ˜ W ) =   1 gH − U2 2U gH ˜ α ˜ β   where ˜ α = ∂Qs ∂H and ˜ β = ∂Qs ∂Q .

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation of the Saint-Venant–Exner equations

Definition of the wave velocities

The main issue comes from the choice of λL and λR. Recall A( ˜ W ) =   1 gH − U2 2U gH ˜ α ˜ β   where ˜ α = ∂Qs ∂H and ˜ β = ∂Qs ∂Q . Characteristic polynomial of A: pA(λ) = λ3 − 2Uλ2 − (gH(1 + ˜ β) − U2)λ − gH ˜ α = 0. (20)

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Numerical approximation of the Saint-Venant–Exner equations

Definition of the wave velocities: Nickalls’ bounds (2011)

Derivative quadratic equation of pA: 3λ2 − 4Uλ − (gH(1 + ˜ β) − U2) = 0. (21)

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation of the Saint-Venant–Exner equations

Definition of the wave velocities: Nickalls’ bounds (2011)

Derivative quadratic equation of pA: 3λ2 − 4Uλ − (gH(1 + ˜ β) − U2) = 0. (21) The solutions are λ± = x0 ± Ω, (22) such as x0 = 2U 3 and Ω = 1 3

  • U2 + 3gH(1 + ˜

β).

  • Ph. Ung

Egrin – Jun. 1st, 2015 Coupling for Sedim. Transp. 23 / 33

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Context & Motivations Numerical scheme Test cases Discussion

Numerical approximation of the Saint-Venant–Exner equations

Definition of the wave velocities: Nickalls’ bounds (2011)

Derivative quadratic equation of pA: 3λ2 − 4Uλ − (gH(1 + ˜ β) − U2) = 0. (21) The solutions are λ± = x0 ± Ω, (22) such as x0 = 2U 3 and Ω = 1 3

  • U2 + 3gH(1 + ˜

β). The wave velocities are defined by λL = x0 − 2 Ω, (23) λR = x0 + 2 Ω. (24)

  • Ph. Ung

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Context & Motivations Numerical scheme Test cases Discussion

Numerical scheme

Summary

Associated Godunov-type scheme

       ˜ W n+1

i

= ˜ W n

i − ∆tn

∆x (F −

i+1/2 − F + i−1/2) ,

˜ W 0

i =

1 ∆x

  • Ci

H0(x)dx,

  • Ci

(H0U0)(x)dx,

  • Ci

B0(x)dx T ,

where F − and F + are given by    F −( ˜ WL, ˜ WR) = F( ˜ WL) + λL

  • ˜

W ⋆

L − ˜

WL

  • ,

F +( ˜ WL, ˜ WR) = F( ˜ WR) + λR

  • ˜

W ⋆

R − ˜

WR

  • ,

and the wave velocities are defined by λL = x0 − 2 Ω, λR = x0 + 2 Ω, with x0 = 2U 3 and Ω = 1 3

  • U2 + 3gH(1 + ˜

β) and ˜ β = ∂Qs ∂Q .

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Context & Motivations Numerical scheme Test cases Discussion

Test cases

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Numerical results

Evolution of a bump in a fluvial regime

Figure: Bump in fluvial (top) and transcritical (bottom) flow.

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Numerical results

Evolution of a bump in a torrential regime

Figure: Antidune.

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Numerical results

Dam break over a wet bed

Figure: Dam break over wet (top) and dry (bottom) topographies.

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Context & Motivations Numerical scheme Test cases Discussion

Discussion

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Context & Motivations Numerical scheme Test cases Discussion

Discussion

Splitting vs non-splitting methods

Figure: Bump on fluvial (left) and transcritical (right) regimes.

  • Ph. Ung

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Discussion

Splitting vs non-splitting methods

Figure: Antidune.

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Discussion

Splitting vs non-splitting methods

Figure: Dam break over wet (top) and dry (bottom) bed.

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Thank you for your attention!

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