On an inverse Cauchy problem arising in tokamaks Yannick Fischer - - PowerPoint PPT Presentation

on an inverse cauchy problem arising in tokamaks
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On an inverse Cauchy problem arising in tokamaks Yannick Fischer - - PowerPoint PPT Presentation

On an inverse Cauchy problem arising in tokamaks Yannick Fischer INRIA Sophia-Antipolis projet APICS joint work with L. Baratchart*, J. Leblond* *INRIA (Sophia-Antipolis) SMAI - 23 Mai 2011 Cauchy problem R 2 : annular domain with


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On an inverse Cauchy problem arising in tokamaks

Yannick Fischer

INRIA Sophia-Antipolis projet APICS joint work with

  • L. Baratchart*, J. Leblond*

*INRIA (Sophia-Antipolis)

SMAI - 23 Mai 2011

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Cauchy problem

Ω ⊂ R2 : annular domain with smooth boundary ∂Ω = Γi ∪ Γe σ : smooth function (Lipschitz) with 0 < c ≤ σ ≤ C ∇ · (σ∇u) = 0 a.e in Ω with u and ∂nu prescribed on I ⊆ ∂Ω Can we recover u and ∂nu on J = ∂Ω \ I ?

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Application to tokamak

Physical motivation : application to Tokamak (Tore Supra)

z r y x ϕ

Axisymmetric configuration (3D-problem) = ⇒ Study of the equilibrium in poloidal section (2D-problem)

z r Γp Γe Γl R ρe Ωp Ωl ρl

Maxwell equation in the vacuum Ωl : ∇.(1 r ∇u) = 0 where u(r, z) is the magnetic poloidal flux and σ = 1

r is regular in

Ωl. How to recover u and ∂nu on Γl from (finite) measurements on Γe ?

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The conjugate Beltrami equation

Idea : Astala and P¨ aiv¨ arinta (2006) From real equation ∇ · (σ∇u) = 0 a.e in Ω (CD) σ ∈ W 1,∞

R

(Ω) to complex equation (but R-linear) ∂f = ν∂f a.e in Ω (CB) ν ∈ W 1,∞

R

(Ω) Proposition f = u + iv ∈ W 1,2(Ω) satisfies (CB) with ν = 1−σ

1+σ

= ⇒ ∇.(σ∇u) = ∇.(σ−1∇v) = 0 a.e in Ω and

  • ∂xv

= −σ∂yu ∂yv = σ∂xu a.e in Ω (or ∂tv = σ∂nu a.e on ∂Ω)

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The conjugate Beltrami equation

Advantages :

  • Symmetric roles played by u and v

Dirichlet + Neumann conditions for u ⇓ Dirichlet condition for u + Dirichlet condition for v =

  • ∂Ω σ∂nu

⇓ ONLY Dirichlet conditions for f

  • Allow regularization of the Cauchy problem for data in L2(∂Ω)
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Generalized Hardy classes

Definition H2

ν(Ω) = Lebesgue measurable fonctions f on Ω such that

f H2

ν(Ω) := ess sup

̺<r<1

  • 1

|f (reiθ)|2dθ

1/p

< +∞ (1) and solving (CB) in the sense of distributions in Ω H2

ν(Ω) is a Hilbert space. When ν = 0 and Ω = D, recover

the classical H2(D) space of holomorphic functions in D satisfying (1) .H2

ν(Ω) ∼ .L2(∂Ω)

tr H2

ν(Ω) is closed subspace of L2(∂Ω)

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Density result

Theorem Let I ⊂ ∂Ω be a mesurable subset such that |I|, |J| > 0 tr H2

ν(Ω)|I is dense in L2(I)

As tr H2

ν(Ω) is a closed subset of L2(∂Ω), if (fk)k≥1 ∈ H2 ν(Ω) is

such that tr fk − f L2(I) − →

k

0, there are only two possibilities : f = (tr F)|I with F ∈ H2

ν(Ω)

  • r

tr fkL2(J) → +∞ This leads to a bounded extremal problem.

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Bounded extremal problems...

If (u, v) are compatible data on I − → unique solution by extrapolation If (u, v) are NOT compatible data on I Idea : constrain solutions on J. Definition For M > 0 and ϕ ∈ L2

R(J)

B =

  • f ∈ tr H2

ν(Ω); f − ϕL2(J) ≤ M

  • |I ⊂ L2(I)

extrapolation problem ← → well-posed L2 approximation problem

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...Bounded extremal problems

Then the approximation problem admits a unique solution Theorem Fix M > 0 ∀f ∈ L2(I), ∃! g0 ∈ B / f − g0L2(I) = min

g∈Bf − gL2(I)

Moreover, if f / ∈ B, then g0 − ϕL2(J) = M The solution g0 is given by g0 = g0(λ) = (I + λPνχJ)−1Pν(χIf ∨ (1 + λ)ϕ) with λ ∈ (−1, ∞).

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Algorithm

plasma boundary = outermost closed magnetic surface in the limiter

1.6 1.8 2 2.2 2.4 2.6 2.8 3 3.2 −0.8 −0.6 −0.4 −0.2 0.2 0.4 0.6 0.8

1) u = N

i=1 αibi from u and

∂nu on Γext 2) u0 = max u on the limiter and Γ1

int = {(x, y); u(x, y) = u0}

∂Ω1 = Γext ∪ Γ1

int

3) BEP in Ω1 ⇒ g0 = min f − g with Re g0 − u0 = M 4) u1 = max Re g0 on the limiter and Γ2

int = {(x, y); Re g0 = u1}

etc...

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Simulations

pi/2 pi 3pi/2 2pi 0.65 0.7 0.75 0.8 0.85 0.9 Θ ρ(m) BEP0_6 EFIT_REF LIM

Fig.: Graphe de θ → ρ(θ) pour les fronti` eres plasma et le limiteur.

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Simulations

pi/2 pi 3pi/2 2pi 0.65 0.7 0.75 0.8 0.85 0.9 Θ ρ(m) BEP0_6 BEP1_6_6 EFIT_REF LIM

Fig.: Graphe de θ → ρ(θ) pour les fronti` eres plasma et le limiteur.

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Simulations

pi/2 pi 3pi/2 2pi 0.65 0.7 0.75 0.8 0.85 0.9 Θ ρ(m) BEP0_6 BEP1_6_6 BEP1_6_10 EFIT_REF LIM

Fig.: Graphe de θ → ρ(θ) pour les fronti` eres plasma et le limiteur.

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Simulations

pi/2 pi 3pi/2 2pi 0.65 0.7 0.75 0.8 0.85 0.9 Θ ρ(m) BEP0_6 BEP1_6_6 BEP1_6_10 BEP1_6_14 EFIT_REF LIM

Fig.: Graphe de θ → ρ(θ) pour les fronti` eres plasma et le limiteur.

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Simulations

pi/2 pi 3pi/2 2pi 0.65 0.7 0.75 0.8 0.85 0.9 Θ ρ(m) BEP0_6 BEP1_6_6 BEP1_6_10 BEP1_6_14 BEP1_6_18 EFIT_REF LIM

Fig.: Graphe de θ → ρ(θ) pour les fronti` eres plasma et le limiteur.

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Conclusion

Fast method (no mesh) compact representation with solutions of the equation evaluation of the poloidal flux between the plasma and the

  • utside boundary

Work in progress : Optimization of the Lagrange parameter λ pathological cases

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Thank you for your attention