cn2 profile measurement from shack-hartmann data

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Cn2 profile measurement from Shack- Hartmann data Clélia Robert, Nicolas Védrenne,Vincent Michau, Jean-Marc Conan

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Cn2 profile measurement from Shack-Hartmann data. Clélia Robert, Nicolas Védrenne,Vincent Michau, Jean-Marc Conan. C n ² ?. C n ² ?. C n ² ?. C n ² ?. C n ² ?. C n ² ?. A new method to profile C n 2. Measurement of C n ² profile. Motivation and techniques Shack-Hartmann data - PowerPoint PPT Presentation

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Page 1: Cn2 profile measurement from Shack-Hartmann data

Cn2 profile measurement from Shack-Hartmann data

Clélia Robert, Nicolas Védrenne,Vincent Michau, Jean-Marc Conan

Page 2: Cn2 profile measurement from Shack-Hartmann data

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A new method to profile Cnn2

Cn² ?

Cn² ?

Cn² ?

Cn² ?

Cn² ?

Cn² ?

Page 3: Cn2 profile measurement from Shack-Hartmann data

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I. Motivation and techniques

II. Shack-Hartmann data

III. Exploitation to measure Cn2 profile

IV. Numerical validation

Measurement of Cn² profile

Page 4: Cn2 profile measurement from Shack-Hartmann data

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Cn2 Profile

Profile from Observatoire de Haute Provence (ballon sonde)

Profile knowledge:

High variability

Need of profilemonitoring

Dimensioning systemsEvaluation of performancesA priori for servo-loop laws

How to measure ?

Page 5: Cn2 profile measurement from Shack-Hartmann data

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MASS (V. Kornilov, A. Tokovinin) SSCIDAR (D. Garnier)

More operations needed(mode: « generalized»)

No sensitivity to law altitude layers (no propagation)

intensité dans la pupille

Spectral analysis of scintillation structures

TF

(λh)-(1/2)

PSDχ(ν)

ν

h

More uncertainties

Principles of Cn2 profiling : single source

Single source: low vertical resolution

Page 6: Cn2 profile measurement from Shack-Hartmann data

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Principles of Cn2 profiling : multiple source

Slopes: Cross-correlations of wavefront slopes: SLODAR (R.W. Wilson)

What about simultaneous exploitation of slopes and intensities ?

h

θ

Intensities: Cross-correlations of scintillation indices: G-SCIDAR (J. Vernin, V.A. Klueckers)

θ X h

Page 7: Cn2 profile measurement from Shack-Hartmann data

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I. Motivation and techniques

II. Shack-Hartmann data

III. Exploitation to measure Cn2 profile

IV. Numerical validation

Measurement of Cn² profile

Page 8: Cn2 profile measurement from Shack-Hartmann data

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Shack Hartmann Wavefront sensor

SH data:

sm(θ) = wavefront slopes averaged on subaperture at rm

im(θ) = averaged intensity of the incident wave on subaperture at rm

m

x

yrm

αα

Page 9: Cn2 profile measurement from Shack-Hartmann data

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Correlations of data (intensities & slopes):

h

Page 10: Cn2 profile measurement from Shack-Hartmann data

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Propagation + subaperture averaging

m

h

rm

Correlations of data (intensities & slopes):

Small perturbation approximation (Rytov regime, σχ

2 < 0.3)

Page 11: Cn2 profile measurement from Shack-Hartmann data

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Propagation + subaperture averaging

θ

m

h

rm θh – rm

Correlations of data (intensities & slopes):

Page 12: Cn2 profile measurement from Shack-Hartmann data

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Propagation + subaperture averaging

dmn

θ

m n

h

Correlations of data (intensities & slopes):

Page 13: Cn2 profile measurement from Shack-Hartmann data

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Propagation + subaperture averaging

dmn

θ

m n

h

θh

Correlations of data (intensities & slopes):

Altitude of maximum sensitivity

Page 14: Cn2 profile measurement from Shack-Hartmann data

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Propagation + moyenne sur la sous-pupille

dmn

θ

m n

h

θh

Correlations of data (intensities & slopes):

unknown WeightingMeasurement

Page 15: Cn2 profile measurement from Shack-Hartmann data

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Correlations of Shack-Hartmann data

Slopes

Coupling

Intensities

SLODAR

SCIDAR, MASS Shack-Hartmann ++ !!

Page 16: Cn2 profile measurement from Shack-Hartmann data

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Complementarity of measurements

D= 0.4 m,16 x 16, λ = 0.5 μm

Simultaneous exploitation: better sensitivity

80 %

15 %

5 %

Slopes Intensities

Se:

dy

n

m

dmn

dx

dy

Shack-Hartmann:

Law layers High layers

sensitivity:

Page 17: Cn2 profile measurement from Shack-Hartmann data

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I. Motivation and techniques

II. Shack-Hartmann data

III. Exploitation to measure Cn2 profile

IV. Numerical validation

Measurement of Cn² profile

Page 18: Cn2 profile measurement from Shack-Hartmann data

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Problem statement

Estimated covariances:

SH data: sm(θ), im(θ): xki

: covariance of detection noise (bias)

: statistical noise on

Direct problem:

: weighting functions

Multiple sourcesSingle source

ou

Pseudo data

Page 19: Cn2 profile measurement from Shack-Hartmann data

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Inversion of direct problem

CalibrationSubtraction of detection

noise bias

Pseudo-data:

Covariance matrixCnoise

Limited statistic(convergence noise)

Noise treatment:

Minimisation of J with positivity constraint

: regularisation parameter (depends on h)

Criterion to minimise relatively to S (Cn2 profile)

-1

Data likelihood A priori

Page 20: Cn2 profile measurement from Shack-Hartmann data

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I. Motivation and techniques

II. Shack-Hartmann data

III. Exploitation to measure Cn2 profile

IV. Numerical validation

Measurement of Cn² profile

Page 21: Cn2 profile measurement from Shack-Hartmann data

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Simulation:

Data: sm(θ), im(θ)

16 x 16, d = 2.5 cm, λ = 0.5 μm (D = 40 cm)Shack-Hartmann:

Object model: binary starθ = 10 arcsec.

Code PILOTSimulation of turbulent screens

+ Diffractive propagation

32 layers/ 400 frames

+

+

Page 22: Cn2 profile measurement from Shack-Hartmann data

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Preliminary results

N. Védrenne, V. Michau, C. Robert, J.-M Conan, « Improvements in Cn2 profile monitoring with a Shack-Hartmann wavefront sensor », Proc. SPIE Vol. 6303,

septembre 2006.N. Védrenne, V. Michau, C. Robert, J.-M Conan, « Full exploitation of Shack-Hartmann data for Cn

2 profile measurement », OL, octobre 2007

Page 23: Cn2 profile measurement from Shack-Hartmann data

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Conclusion and perspectives:

Proposition of two original methods to profile Cn2

New exploitation of the Shack-Hartmann

Sensitivity

Validated numerically

Study of nois effect (photons, detector, quantification)

Processing of real data (SLODAR)

Determination of wind profile

Calibration

Adaptation to close binary, moon edge, sun edge

Influence of external scale?