Géraldine Guerri Post-doc CSL

Slides:



Advertisements
Similar presentations
Fast & Furious: a potential wavefront reconstructor for extreme adaptive optics at ELTs Visa Korkiakoski and Christoph U. Keller Leiden Observatory Niek.
Advertisements

Optical Testing for Next Generation Optical Telescopes; Terrestrial and Space Robert E. Parks Optical Perspectives Group, LLC Tucson, AZ September, 2002.
kHz-driven high-harmonic generation from overdense plasmas
SLAC National Accelerator Center
October 10th, 2007Osservatorio Astrofisico di Arcetri1 Application of the pyramid wavefront sensor to the cophasing of large segmented telescopes F. Quirós-Pacheco,
Vision and Revision Wavefront Sensing from the Image Domain Benjamin
1 Laser Beam Coherence Purpose: To determine the frequency separation between the axial modes of a He-Ne Laser All sources of light, including lasers,
FLAO Alignment Procedures G. Brusa, S. Esposito FLAO system external review, Florence, 30/31 March 2009.
Adaptive Optics for Wavefront Correction of High Average Power Lasers Justin Mansell, Supriyo Sinha, Todd Rutherford, Eric Gustafson, Martin Fejer and.
Optical Alignment with Computer Generated Holograms
The Linear Collider Alignment and Survey (LiCAS) Project Richard Bingham*, Edward Botcherby*, Paul Coe*, Grzegorz Grzelak*, Ankush Mitra*, Johannes Prenting.
1 Experimental determination of K I by Annex IV Speckle interferometry.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Green Bank Laser Rangefinders.
Thermally Deformable Mirrors: a new Adaptive Optics scheme for Advanced Gravitational Wave Interferometers Marie Kasprzack Laboratoire de l’Accélérateur.
High index glass spherical targets for laser interferometry Miroslav Sulc 1st PACMAN worshop 1.
Telescope Errors for NGAO Christopher Neyman & Ralf Flicker W. M. Keck Observatory Keck NGAO Team Meeting #4 January 22, 2007 Hualalai Conference Room,
Figuring large off-axis segments to the diffraction limit Hubert Martin Steward Observatory University of Arizona.
ASTRI SST-2M The Prototype monolithic 1.8 m
Page 1 Lecture 3 Part 1: Finish Geometrical Optics Part 2: Physical Optics Claire Max UC Santa Cruz January 15, 2012.
Single-shot characterization of sub-15fs pulses with 50dB dynamic range A. Moulet 1, S.Grabielle 1, N.Forget 1, C.Cornaggia 2, O.Gobert 2 and T.Oksenhendler.
Cophasing activities at Onera
Blue Dot Team « Multi aperture imaging ». BDT sept MAI techniques High accuracy visibility measurement Differential interferometry Nulling.
8 September Observational Astronomy TELESCOPES, Active and adaptive optics Kitchin pp
Volumetric 3-Component Velocimetry (V3V)
MCAO Adaptive Optics Module Subsystem Optical Designs R.A.Buchroeder.
The Michelson interferometer Best known and historically most important Best known and historically most important Utilizes arrangement of mirrors (M)
LSC meeting, HLO, August 18, 2004 IAP/UF/LIGO Research Collaboration: Status and Prospectives Efim Khazanov, Ilya Kozhevatov, Anatoly Malshakov, Oleg Palashov,
Laboratory prototype for the demonstration of sodium laser guide star wavefront sensing on the E-ELT Sexten Primary School July 2015 THE OUTCOME.
19 February 2009 Cophasing sensor for synthetic aperture optics applications First steps of the development of a cophasing sensor for synthetic aperture.
IPBSM status and plan ATF project meeting M.Oroku.
Scatterfield Zero Order Imaging
BROOKHAVEN SCIENCE ASSOCIATES BIW ’ 06 Lepton Beam Emittance Instrumentation Igor Pinayev National Synchrotron Light Source BNL, Upton, NY.
Tomographic reconstruction of stellar wavefronts from multiple laser guide stars C. Baranec, M. Lloyd-Hart, N. M. Milton T. Stalcup, M. Snyder, & R. Angel.
FLAO system test plan in solar tower S. Esposito, G. Brusa, L. Busoni FLAO system external review, Florence, 30/31 March 2009.
1 1 st Light AO 4 LBT Pyramid WFS Adaptive Secondary MMT Unit.
Page 1 Adaptive Optics in the VLT and ELT era François Wildi Observatoire de Genève Credit for most slides : Claire Max (UC Santa Cruz) Optics for AO.
The Hobby-Eberly Telescope Mirror Alignment Recovery System Marsha Wolf Graduate Student UT Astronomy Department.
1/30 Challenge the future Auto-alignment of the SPARC mirror W.S. Krul.
1 High-order coronagraphic phase diversity: demonstration of COFFEE on SPHERE. B.Paul 1,2, J-F Sauvage 1, L. Mugnier 1, K. Dohlen 2, D. Mouillet 3, T.
Zero field The 25 ‑ m f /0.7 primary mirror for the Giant Magellan Telescope (GMT) is made of seven 8.4 ‑ m segments in a close packed array. Each of the.
1 Design and analysis for interferometric measurements of the GMT primary mirror segments J. H. Burge a,b, L. B. Kot a, H. M. Martin a, R. Zehnder b, C.
Optical principles of diffraction focussing, Preparing the way to space borne Fresnel imagers NiceSeptember 23-25, Fresnel Imagers Observatoire.
T. Suehara, H. Yoda, T. Sanuki, Univ. of Tokyo, T. Kume, Y. Honda, T. Tauchi, High Energy Accelerator Research Organization (KEK) ATF2-IN2P3-KEK kick-off.
Large Dynamic Range Co- Phasing System Development for Segmented Telescope Mirrors Juan F Simar – ARC Phd Student Centre Spatial de Liège Université de.
Osservatorio Astronomico di Padova A study of Pyramid WFS behavior under imperfect illumination Valentina Viotto Demetrio Magrin Maria Bergomi Marco Dima.
Pre-focal wave front correction and field stabilization for the E-ELT
Hartmann Sensor for advanced gravitational wave interferometers
The Self-Coherent Camera: a focal plane wavefront sensor for EPICS
IFS prototype – PM3 LAM, 13/06/2003 Prototype testing at CRAL Tests at room temperature in the visible.
Adaptive Optics in the VLT and ELT era Optics for AO
J. H. Burgea,b, W. Davisona, H. M. Martina, C. Zhaob
Parameters characterizing the Atmospheric Turbulence: r0, 0, 0
Optomechanical Technologies for Astronomy, SPIE 6273 (2006)1 Manufacture of a 1.7 m prototype of the GMT primary mirror segments Buddy Martin a, Jim Burge.
Large Dynamic Range Co-Phasing System Development for Segmented Telescope Mirrors Piston and Tip/Tilt expected errors The initial error after deployment.
Parc Kennedy - Bat A , Rue Gilles Roberval / F NIMES  +33 (0) /  +33 (0) / Web :
Midterm Review 28-29/05/2015 Progress on wire-based accelerating structure alignment Natalia Galindo Munoz RF-structure development meeting 13/04/2016.
Progress of Shintake Monitor (ATF2 IP-BSM) ATF2 weekly meeting 2008/9/3 Takashi Yamanaka The University of Tokyo.
Tip/tilt options Trade Study Report on Stand-alone T/T vs. DM on T/T Stage (WBS ) Brian Bauman December 12, 2006.
Smart co-phasing system for segmented mirror telescopes SPIE: Juan F Simar* a, Yvan Stockman a, Jean Surdej b a Centre Spatial de Liège, LIEGE.
Design and Manufacture of a Large Aperture Wavefront Sensor (LAWS)
Carousel Interferometer for Metrological Applications
Pre-launch Characteristics and Calibration
Pyramid sensors for AO and co-phasing
Extended Scene Shack-Hartmann
Interferometric measurements on mirrors
Digital Holographic Microscopy for Quantitative Visualization
Deflectometry-based Measurement And Correction Of Mirror Misalignment
*School of Computer and Information, Hefei University of Technology
Optics Alan Title, HMI-LMSAL Lead,
Calibration Plan Chris Neyman W. M. Keck Observatory April 20, 2010.
Presentation transcript:

Géraldine Guerri Post-doc ARC @ CSL 4 March 2011 First results of the CSL piston sensor breadboard and further application Géraldine Guerri Post-doc ARC @ CSL Liège Space Center, Angleur 4 March 2011

Framework : Extremely Large Telescopes (ELT) On the ground : In space : JWST : 18 segments, 6.5m aperture, 25 kg/m² density Increasing demand for larger apertures : 20m diameter, 3 kg/m² density E-ELT (Europe) 42 m diameter 1000 segments GMT (USA) 25 m diameter 7 segments TMT (Europe) 30 m diameter 492 segments Géraldine Guerri 4 March 2011 2

Large lightweight space telescope Technological need : Critical issues : manufacturing wavefront error control sub-aperture coherent alignement CSL concern : Developpement of demonstrator breadboard of a cophasing sensor for space segmented mirrors made with 3 or 7 segments large diameter deployable lightweight cheap space mirrors Géraldine Guerri 4 March 2011 3

What is a cophasing sensor ? Measure the relative positioning of each subaperture : determination of piston and tip-tilt errors Piston : Translation along the optical axis (λ or nm) 2 phasing regimes : Coarse phasing in open loop Fine phasing in closed loop : error < λ/2 Tip/ Tilt : Rotation of the sub-pupil perpendicular to the optical axis (rad or arsec) Géraldine Guerri 4 March 2011 4

Sensor requirements Cophasing of 3 to 7 sub-apertures Separate measurement of piston and tip/tilt Low weight and Compacity Real-time correction Reduced hardware complexity Linearity, High range and accuracy Piston measurement Tip/tilt measurement Range: ± 1 mm Range: 100 µrad Accuracy: 0.5 µrad Accuracy: 50 nm Géraldine Guerri 4 March 2011 5

Cophasing sensor architecture PISTON TIP-TILT COARSE PHASING Cf JF Simar presentation FINE COPHASING Error < λ/2 Phase retrieval real-time algorithm (Baron et al., 2008) Shack-Hartmann Sensor or Phase diversity real-time algorithm (Mocoeur et al., 2008) Géraldine Guerri 4 March 2011 6

Why phase retrieval technique ? Phase error extracted from one focal image Baron et al., 2008 : For fine cophasing (error < λ/2), analytical and real-time solutions exists Only ONE FFT computation needed Object Focal plane image Phase retrieval algorithm ? Géraldine Guerri 4 March 2011 7

Phase retrieval algorithm Without Piston error Differential Piston errors can be determined from the intensity of peaks of the phase of the OTF OTF Modulus OTF Phase PSF 3 aperture pupil With Piston error Géraldine Guerri 4 March 2011 8

Piston sensor validation breadboard Géraldine Guerri 4 March 2011 9

Piston sensor breadboard optical setup Laser He-Ne λ= 633 nm P1 Creation of collimated beam O1 3 sub-apertures Pupil mask These mirors reflect only 2 sub-pupils over 3 MP M4 M5 Delay line to compensate the OPDs between the 2 paths M1 M2 M3 L1 O2 M6 CCD PZT S1 Miror + PZT : Introduction of a piston error on 1 sub-aperture Beamsplitter : re-formation of the pupil with 3 sub-apertures Piston sensor components Géraldine Guerri 4 March 2011 10

Piston sensor experimental results Application of a piston ramp on a sub-aperture : Géraldine Guerri 4 March 2011 11

Piston sensor experimental results Metrological standards obtained from measurements : Results presented at SPIE conference « Astronomical Telescopes and Instrumentation 2010 » Measurement range [ -λ/2 , λ/2 ] Linearity >0.92 (best 0.96) Resolution < 20 nm Deviation around zero point < 10 nm Absolute error ±25 nm Géraldine Guerri 4 March 2011 12

Feedbacks from experimental tests Dependance of the phase measurements accuracy on : the wavefront error of each beam until the common path (<λ/10 rms) the set-up stability (vibration and drift during the measurement) the PSF pattern (‘‘fringe’’) contrast The beam coherence The image quality of the imaging lens Géraldine Guerri 4 March 2011 13

Future prospects Experimental feasibility tests of the Phase Retrieval technique with a 7 sub-apertures system Study and design of a system to introduce various and precise piston values Design and implementation of the coarse piston sensor (cf JF Simar PhD) Design and implementation of the tip-tilt measurement Géraldine Guerri 4 March 2011 14

Application Cophasing of 3 silicon bimorph mirors developed at ULB (Rodrigues et al., 2009) Géraldine Guerri 4 March 2011 15

Cophasing demonstrator principle 3 segments deformable mirror demonstrator Collimated beam (Φ=130mm) Piston sensor Illuminating system Géraldine Guerri 4 March 2011 16

Optical simulation of the cophasing demonstrator Development of an end-to-end simulation (Matlab, ASAP) Illuminating system Piston sensor Illuminating system 1 pupil mask with 3 sub-apertures 1 beamsplitter (90/10) 1 pupil imaging camera 1 imaging lens 1 focal image camera 1 computer 1 He-Ne Laser (λ=633 nm) 1 Microscope objective 1 Pinhole (Φ=15 µm) 1 Off-axis parabola Piston sensor Géraldine Guerri 4 March 2011 17

3 segment cophasing demonstrator Calibration tests in progress in Liège … Validation tests in Bruxelles very soon .. Illuminating system Piston sensor Géraldine Guerri 4 March 2011 18

Thanks for your attention Géraldine Guerri 4 March 2011 19

3 segment cophasing demonstrator 3 segments mirror Illuminating system Piston sensor 1 pupil mask with 3 sub-apertures 1 beamsplitter (90/10) 1 pupil imaging camera 1 imaging lens 1 focal image camera 1 computer 1 He-Ne Laser (λ=633 nm) 1 Microscope objective 1 Pinhole 1 Off-axis parabola Calibration tests in progress in Liège… Validation tests in Bruxelles very soon Géraldine Guerri 4 March 2011 20

Géraldine Guerri 4 March 2011 21

Sensor techniques selection Work plan Survey of state of the art of cophasing sensor Sensor techniques selection Validation by numerical simulations Experimental validation Feasibility demonstrator of the cophasing of 3 sub-apertures with standard optical components Study and Design of a space-compatible breadboard Géraldine Guerri 4 March 2011 22

Géraldine Guerri 4 March 2011 23