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MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics: F. Guglielmetti, R. Fischer, V. Dose, MaxEnt Proceedings 2004, p.111-118

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

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Page 1: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 1

Udo v. Toussaint, Silvio Gori

2-D Deconvolution

using

Thin-Plate Splines

Astrophysics: F. Guglielmetti, R. Fischer, V. Dose, MaxEnt Proceedings 2004, p.111-118

Page 2: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 2

Fusion research and Bayes

Fusion research:

• Huge number of diagnostics

• Complementary information

• Long operation time (decades)

Synergism by exploiting full probabilistic correlation structure of

diagnostics: Integrated Data Analysis

Possibility of Experimental Design

Perfectly suited for Bayesian Analysis:

Page 3: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 3

Fusion Research

Example: W7-X

Thomson scattering

ECE

Magnetics

Langmuir Probes

Interferometry

Bolometry

Video

H

Calorimetry

Neutral gas

Vis. spectroscopy

CXRS

SPRED

Soft-X ray

Thermography

Flux surface measurements

Diagnostic beam

Neutron detectors

Diagnostics Software(data analysis)

General purpose (stellarator) software

Integrated data analysis

Modelling

Infrastructure &management

Spectroscopy

Imaging

Tomography

DedicatedDiagnostics(misc.)

W7-X DiagnosticsSoftware

2-D diagnostics essential!

BES

Zeff

CO-Monitor

(by A. Dinklage)

Page 4: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 4

Fusion Research: Tomography

Wide variety of tomographic configurations: experimental requirements, costs,…

Goal: best possible reconstruction of 2-D profile

Page 5: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 5

Fusion Research: Tomography

•Tomographic reconstruction: underdetermined & ill-posed

• Prior information available

standard inversion techniques

mostly perform poorly

??

?

??

? ??

?

Page 6: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 6

Thin-Plate Splines

-Transport along magnetic field lines very fast: smooth profiles usually favored:

curvature only when enforced by the data

- 1D- case: cubic splines

- 2D- case: Minimize curvature IB of f(x,y) (can be generalized )

222 2 yyxyxxB fffdydxI

Fundamental solution[1]:

22 ln rrrU

[1] G. Wahba, Spline models for Observational Data, SIAM, 1990

Page 7: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 7

Thin-Plate Splines

Interpolating function z=f(x,y):

3,||,,||, 01

nyaxaayxyxUwyxfz yxii

n

ii

Coefficients wi, a are given by the solution of

00

z

a

w

P

PKT

with Kij=U(||(xi,yi)-(xj,yj)||), Pi=(1,xi,yi)

The bending energy is given by zrwwKwwI TB ,,

Page 8: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 8

Model

Model: jj

iji gCm , Cij: response matrix

gj : emissivity on grid space

Likelihood: 2

2

2,,|

i

iiii

mdIgdp

with ),( yxfdxdygjA

j

Page 9: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 9

)|(,|),,|()|( InpInRpInRzpIMp

)),(),(exp(1

,,| zRwKzRwZ

nRzp T

!)3(

!)!()|,(

NN

nnNInRp

Prior Distributions

• Number of support points n on grid with N places:

• Curvature : Testable information

• Hyperparameter :

MaxMinIp ,/1)|(

• Model prior factorizes:

Page 10: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 10

IpIRzpdIRzDpzdIMp

IRzpIRzDpzdIMpIMDpIMpIDMp

|,,|,,||

,|,,||,||,|

Posterior

• Posterior for Model Mi :

• Evidence approximation:

• Simple sampling in N,R

• 1-D search in : *

2/1**** )det(,|,,,,|,| HIMzpIMzDpIMDp

)det(

)2(,,|,,,||

,,|,,||,,|

0

**

HIMzpIMzDpIp

IMzpIMDpzdIpIMDp

n

• Optimization preferred: Laplace Approximations…

Page 11: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 11

Thin-Plate Splines: Results

• Reconstruction of challenging (but realistic) 2-d emission profile:

• Result of evidence weighted average

Mock profile: Reconstruction: Difference:

Key features, shape and absolut intensity recovered

Page 12: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 12

Thin-Plate Splines: Results

Location of z-optimized support points:

Open issue: Support points outside of region of interest beneficial?

Reconstruction within the uncertainty

Page 13: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 13

Thin-Plate Splines: Outlook

• Extension to f(x,y,z): Viewing cone

• Extension to f(x,y,(z),t):

time correlated data

Connection to morphing applications

Drawback: Huge amounts of data to be processed

• Online (monitoring) requirements:Use as input for Bayesian Neural Networks

• Check approximations with MCMC

Page 14: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 14

Thin-Plate Splines: Conclusion

Thank you!

Page 15: MaxEnt 2007, Udo v. Toussaint, July 2007, udo.v.toussaint@ipp.mpg.de 1 Udo v. Toussaint, Silvio Gori 2-D Deconvolution using Thin-Plate Splines Astrophysics:

MaxEnt 2007, Udo v. Toussaint, July 2007, [email protected] 15

W7-X: Design

• 50+36SL-Coils

• Optimized shape

• stability without current-drive

• Size:

major: 5.5m

minor: 0.53m

• Magnetic field:

3.3T (2.5T reg)

12kA, 38MW/m2

• Heating:

10 MW ECR

4 MW ICR

5 MW NBI