Survey
* Your assessment is very important for improving the work of artificial intelligence, which forms the content of this project
* Your assessment is very important for improving the work of artificial intelligence, which forms the content of this project
OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA Jean-Marie MACKOWSKI Université Claude Bernard Lyon 1 SMA-VIRGO Bât 213 22, Bd Niels Bohr 69622 Villeurbanne Cedex [email protected] Phone : + 33 04 72 43 26 69 Fax : + 33 04 78 89 19 36 NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA TODAY MENU COATING DEPOSITION TECHNIQUES VIRGO EXPERIENCE VIRGO METROLOGY & OPTICS PERFORMANCES LIMITATIONS SOURCES NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA TODAY MENU COATINGS DEPOSITION TECHNIQUES NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA ION ASSISTED DEPOSITIONAD substrat coating Vapor flow Assistance source material crucible Electron beam, Joule effect, Laser, … NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA I.B.S. Deposition Principles Sample Holder Assist Source O2 + + - Ar Neutralizor - - + + - + - ( Planetary Motion ) + Substrates (Filament, PBN) Targets Meissner Trap NATO/ASI and Euro Summer School September 16-27, 2002 Quartz Sputtered Particles + + + - O2 - + + - - + + - - Neutralizor Sputtering Source Ar Ar JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA I.B.S. Deposition Systems NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA C.V.D Plasma Deposition Systems NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA FROM SOURCE TO SUBSTRAT SURFACE Vapor flow: nature, direction, energy Source Temperature Emission law Substrat Medium pressure Temperature Evaporation: 0.1 eV (1100K) m.s-1 Sputtering: 10 to 50 eV km.s-1 NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO LARGE COATER •Dimension: 2x2.2x2.2 m3 •Vacuum: 2.10-8 mBar •DIBS technology •Environment: Class 1 NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA CLASS 1 CLEAN ROOM BEFORE INTEGRATION NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO LARGE COATER NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA COATING THICKNESS UNIFORMITY •6.10-3 without masking on f 350 mm •3.10-3 with masking on f 700 mm C 01035 C 01041 C 01043 C 01047 PC=50° PC=50° Mask 1 PC=50° Mask 2 PC=50° Mask 3 Thickness uniformity (%) Ta2O 5 5 0 -5 -10 -15 -20 -25 -400 -300 -200 -100 0 100 200 300 400 Position (mm) NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA CORRECTIVE COATING Source Ion d’ions Source SiO2 Cible Target SiO2 Mask Masque Atomes Sputtered Sputtered pulvérisésAtoms Atomes Robot Robot Y X Miroir Mirror Interféromètre Interferometer Contrôle du front d’onde NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA before correction CORRECTIVE COATING 30 nm P.V. 6 nm R.M.S 0 after correction 14 nm P.V. 1.5 nm R.M.S. 0 NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA IBS COATER Absorption @ 1064 nm : 0.2 / 1 ppm Process Difffusion @ 1064 nm : 0.6 / 4 ppm Centring Wavelength repeatability : +/- 0.4 % Wavefront after Corrective Coating : <1 nm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA TODAY MENU VIRGO EXPERIMENT NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO FRANC0-ITALIEN PROJECT 11 Laboratories 5 in France 11 in Italy 200 people 100 M€ Antenna Located at PISA NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO INTERFEROMETER ME1 MIRROR HR R=0.99995 3 km MIRROR R=0.88 MI1 MR MI2 B.S. BS R=0.5 3+ LASER YAG:Nd 20 W AR -4 R<5.10 AR -4 R<5.10 AR -3 R<10 MIRROR R=0.92 AR -4 R<5.10 MIRROR R=0.88 3 km ME2 MIRROR HR R=0.99995 DETECTOR détecteur NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO SITE NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO TUNNEL NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA VIRGO CENTRAL BUILDING W N NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA NATO/ASI and Euro Summer School September 16-27, 2002 VIRGO SUSPENSIONS JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA Beam splitter NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA TODAY MENU VIRGO METROLOGY & OPTICS PERFORMANCES NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA FIRST VIRGO MIRROR • Bulk diameter : 350 mm • Coating diameter : 330 mm • Bulk Thickness : 96 mm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS OPTICS IN ASTROPHYSICS IN ASTROPHYSICS Coatings Coatings Performances Performances & Limitations & Limitations SMA NATO/ASI and Euro Summer School September 16-27, 2002 METROLOGY JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA ABSORPTION BENCH Mesurement of the coating absorption … … as well as the bulk absorption 28W CW YAG:Nd3+ pump laser Mappings up to Ø400 mm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA COATING ABSORPTION (VEM04) @ 1064 nm on Ø 150 mm 0,63 0.07 ppm Ø 150mm Sensitivity: 20 ppb NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA BULK ABSORPTION (VIM03) @ 1064 nm on Ø 150 mm 0,74 0.05 ppm.cm-1 Ø 150mm Sensitivity: 30 ppb.cm-1 NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA BIREFRINGENCE BENCH Mesurement of the amplitude as well as the principle axis direction. Mappings up to Ø400 mm. losses due to birefringence in P or S polarisation (log10) NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA BIREFRINGENCE (VIM01) on Ø 150 mm Amplitude. Sensitivity: 10-5 rad.cm-1 NATO/ASI and Euro Summer School September 16-27, 2002 Principle axis direction JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA RELATIVE REFLEXION BENCH SENSITIVITY: dR/R = 2.10-5 NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA WAVE FRONT MEASUREMENT NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA WAVE FRONT (VEM04) on Ø 150 mm 3.8 mn RMS 29 nm PV Ø 150mm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA STITCHING NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA STITCHING WAVE FRONT (VEM04) on Ø 280 mm 11.6 mn RMS 73.8 nm PV Ø 280mm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA SCATTERING MEASUREMENT Multiplexeur Electronique Platine Goniométrique Détecteur Réflexion Spéculaire Miroir de Focalisation S Echantillon Iris d'alignement Lumière Diffusée Filtre Spatial Modulateur Laser (He-Ne, Yag, CO2) NATO/ASI and Euro Summer School September 16-27, 2002 Détecteur de référence Iris d'alignement M1 M2 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA SCATTERING (VEM04) on 150150 mm2 75 37.5 4 ppm 150150 mm2 0 - 37.5 -75 -75 NATO/ASI and Euro Summer School September 16-27, 2002 - 37.5 0 37.5 75 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA TRANSMISSION (VEM04) on 150150 mm2 42.9 0.2 ppm Ø50mm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA MICROMAP NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA END MIRROR (VEM04) OPTICAL PERFORMANCES SIDE B measurements VIRGO requirements average scattering < 5 ppm 4 ppm 150150 mm2 average transmission 10 < T < 50 ppm 42,9 +/- 0,2 ppm 50 mm average absorption < 5 ppm 0,63 +/- 0,07 ppm 150 mm birefringence -4 < 5.10 SMA-VIRGO measurements -1 rad.cm < 5.10-4 rad.cm-1 150 mm wave front flatness < 8 nm RMS 150 mm 3,8 nm RMS 150 mm shape concave 3450 +/- 100 m 150 mm concave 3580 +/- 17 m f150 mm NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA TODAY MENU LIMITATION SOURCES OF PERFORMANCE NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA LIMITATION SOURCES MATERIALS PURITY SUBSTRATE (BULK) CHEMICALS USED FOR THE POLISHING PROCESS CHEMICALS USED FOR THE CLEANING PROCEDURE SPUTTERING TARGETS COATER WALLS ION SOURCES COMPONENTS GAZ USED FOR DEPOSITION PROCESS, … ENVIRONNEMENTAL CONDITIONS PARTICULATE CONTAMINATIONS ORGANIC CONTAMINATIONS BOXES FOR TRANSFERT & TRANSPORTATION NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA LIMITATION SOURCES MATERIALS PURITY & ENVIRONNEMENTAL CONDITIONS CONTROL PHYSICO-CHEMICAL ANALYSIS TOOLS LIKE : ESCA, RBS, AUGER, SEM, XTM, SIMS… NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA SIMS PRINCIPLES Acquisition Magnetic Quadrupole Scintillator Electron beam (flood gun) Secondary Ions m/e e- Common Ions Sources SAMPLE NATO/ASI and Euro Summer School September 16-27, 2002 O+, Ar+, Cs+, Ga+… JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA MIRRORS :SIMS PROFILES 1,E+05 Oxyde 1 1,E+04 SiO2 Ta205 23 Na Na+ + 23 K + 39 Oxyde 2 intensité (u.a.) K+ 39 1,E+03 1,E+02 1,E+01 1,E+00 0 0,1 0,2 0,3 profondeur (µm) NATO/ASI and Euro Summer School September 16-27, 2002 0,4 0,5 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA MIRRORS :SIMS PROFILES Ta+ NATO/ASI and Euro Summer School September 16-27, 2002 Si+ Ti+ JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA MIRRORS :SIMS PROFILES NATO/ASI and Euro Summer School September 16-27, 2002 JM.M OPTICS IN ASTROPHYSICS Coatings Performances & Limitations SMA CONCLUSION AT THIS STEP, OPTICAL LOSSES IMPROVEMENT NEEDS BIG R&D EFFORTS NATO/ASI and Euro Summer School September 16-27, 2002 JM.M