Corrugated Mirror and Rapid Panel Manufacturing

Slides:



Advertisements
Similar presentations
Global Supply Chain Procurement and Distribution
Advertisements

TMT.OPT.PRE DRF011 Thirty Meter Telescope Secondary and Tertiary Mirror Systems International Symposium on Photoelectronic Detection and Imaging.
Syntec Technologies: Pushing the Polymer Envelope HRDT™ and patent-pending High Refraction Diamond Turning are trademarks of Syntec Technologies.
Optimize Global Shipments with Customized Dunnage Solutions
Announcements Exam 2 is scheduled for two weeks from today (April 2) but, due to all the missed days it will be pushed back one week to April 9 Homework:
M2 Assembly and Feed Optics Ron Price August 25, 2003.
Optics for Photo-Visual Alt-Az Telescopes Dallas Workshop Dave Rowe October 27, 2007.
Multipole Girders - Alignment & Stability (Multipole Girder Alignment technology & R&D) S. Sharma ASD: J. Skaritka, D. Hseuh, V. Ravindranath, G. Miglionico,
Wide-field, triple spectrograph with R=5000 for a fast 22 m telescope Roger Angel, Steward Observatory 1 st draft, December 4, 2002 Summary This wide-field,
NorCal Tech 2005 Technical Conference
Telescopes. Optical Telescopes Ground based and on satellites Observations are recorded using a camera instead of the human eye most times. – This is.
Figuring large off-axis segments to the diffraction limit Hubert Martin Steward Observatory University of Arizona.
Large ‘very’ thin mirror making Why you should use thick glass!
ATLAS Pixel Detector October 2001 Pixel Week N. Hartman LBNL 1 PST Design Update PST CDR october 2001.
Scaling Down - The Optimal Choice? Fritz B. Prinz Departments of Mechanical Engineering and Materials Science and Engineering Stanford University Stanford,
W.O. Miller i T i VG 1 Example Barrel Structures- Disk Primary FEA of Disk Frame Supports FEA of Disk Frame Supports –Structure 2m long with two end plates.
ZTFC 12-segment field flattener (and related) options R. Dekany 07 Aug 2012.
Telescopes Instrument to gather as much EMR as possible and concentrate it into a focused beam. Optical telescopes gather visible light. Other telescopes.
Integral Field Spectrograph Eric PRIETO CNRS,INSU,France,Project Manager 11 November 2003.
High Throughput Microscopy
K-D-PR Fabrication and testing of KGMT FSM prototype Oct Ho-Soon Yang, Hak-Yong Kihm, Il-Kwon Moon, Jae-Bong Song, Yun-Woo Lee Korea.
3.1 Optomechanical systems (1) Scientific and engineering resources are available to carry out the optomechanical work on DECam. The highly distributed.
ZTF Optics Design P. Jelinsky ZTF Technical Meeting 1.
Design of a Lightweight Mounted Tip/Tilt Mirror
Art 12 x 10 Measure art, i.e. 12 x 10 Measure Face (width) of molding i.e. 1 ½ wide Add width of Art (12) + 2 x width of Frame (3) = 15 inches + 1/8 inch.
ZTF Field Flattener 12 segment designs 22 mm thick window P. Jelinsky 2012/11/27.
Absolute Calibration of Null Correctors Using Dual-Computer- Generated Holograms (CGHs) Proteep Mallik, Jim Burge, Rene Zehnder, College of Optical Sciences,
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.
Réunion de présentation des besoins 10 Nov Joël MICHAUD French expertise in SiC for large telescopes.
Specimens are measured in microns (µm)! 1 millimeter = 1000 microns (micro meters) If this caterpillar is 20mm long, how many microns is it? (20mm)(1000)
Design and Development of the FSM (Fast steering Secondary Mirror)
Nanotechnology The Next Big Idea?. Overview ● What is nanotechnology? ● Examples ● Requirements ● Pros and cons ● Conclusion Branched Electron Flow.
LBT Q Engineering Review SAB Static Balancing.
1 Manufacturing Projects Flexible Manufacturing Copyright © Texas Education Agency, All rights reserved.
Jeff Bolognese p1 Super Nova/Acceleration Probe 16 November 2001 Structural Analysis Jeff Bolognese 16 November 2001.
ZTF Optics Design ZTF Technical Meeting 1.
Mass Simulator Concepts Robert Besuner 12 October 2005.
The MesoMill™ An Off-The-Shelf Small Milling Machine By Roger Cortesi MIT Precision Engineering Research Group.
Rapid Prototyping Introduction
Lightweight mirror technology using a thin facesheet with active rigid support J. H. Burge, J. R. P. Angel, B. Cuerden, H. Martin, S. Miller University.
P. Friedrich, H. Bräuninger Extrapolation of the electroforming replication technique as it has been successfully applied to the XMM-Newton mirror systems.
ZTF Field Flattener 12 segment designs P. Jelinsky 2012/10/02.
Optomechanics Lab Presentation OPTI 521L, Fall 2015 Daniel Millstone Kerry Nierenberg.
J. H. Burgea,b, W. Davisona, H. M. Martina, C. Zhaob
다양한 창문을 통한 우주 내용 왜 다양한 창문 ? 왜 다양한 창문 ? 대기의 영향 대기의 영향 망원경의 성능 망원경의 성능 관측에서 얻는 정보 관측에서 얻는 정보 중요 망원경들 중요 망원경들 차세대 망원경들 차세대 망원경들.
LIGO-G D Core Optics Components (COC) Polishing Pathfinder Kickoff Advanced LIGO Project GariLynn Billingsley Caltech.
Some Unusual Telescope Designs Dave Shafer David Shafer Optical Design.
13,14 July 2005 Feasibilty/Concept Study Mid Term Status Review CCAT Enclosure Nathan Loewen AMEC Dynamic Structures Ltd. 13 July 2005.
Material Downselect Rationale and Directions Gregory Harry LIGO/MIT Kavli Institute for Astrophysics and Space Technology On behalf of downselect working.
DESIGN AND DEVELOPMENT OF GRINDING ATTACHMENT ON LATHE MACHINE
A Tour of the Largest Ground-Based Telescopes Being Developed
CCAT Primary Mirror Panel Study
Resource Loaded Schedule and Budget Profile
David Woody Caltech Owens Valley Radio Observatory
The GMT Project The Giant Magellan Telescope (GMT)
THE COMPANY OPTIKRON, your partner for micro-optics, assemblies and optical coatings was founded in 1992 in the optics and technology region of Jena. We.
Scintillators and sensors
Primary Mirror (Reflector)
Laser Beam Welding LIGHT AMPLIFICATION by STIMULATED EMISSION of RADIATION. Coalescence of heat is produced by the Laser beam which is having high energy.
Rapid Prototyping Introduction
Composite Mirror Applications, Inc
Slicer development Eric Prieto LAM.
status of the second field cage
Feasibilty/Concept Study Mid Term Status Review
DESIGN OF CONSTRAINT LECTURE
Rapid Prototyping Introduction
19th Coherent Laser Radar Conference
LSST Camera Detector Status
Scintillators and sensors
Optics Alan Title, HMI-LMSAL Lead,
Presentation transcript:

Corrugated Mirror and Rapid Panel Manufacturing presents Corrugated Mirror and Rapid Panel Manufacturing The Glass Replication Approach to CCAT 13,14 July 2005 Feasibilty/Concept Study Mid Term Status Review

ITT Industries Space Systems Division Heritage Programs 1.8M Keck Telecope (Hawaii) 81 segments 11M Salt (South Africa) 97 segments 11M Hobby-Eberly Telescope (Texas) 96 segments Hubble Space Telesope 1.8M AMSD Off axis asphere 1.4M

Corrugated Mirror Manufacturing Process Sheet Stock Corrugate Core Fuse Assembly Replicate Mandrel Surface Test

Corrugated Glass Mirror Components From Flat Sheet Glass to Corrugated Glass Core (1 Day) 1½-Inch Deep X 1½ Wide “Macro Corrugation” ¼-Inch Deep X 0.2-Inch Wide “Micro Corrugation”

Corrugated Mirror Assemblies Fuse top and bottom plates to corrugated core (1 day) Lightweighting efficiently stiffens face sheets.

Corrugated Mirror Assemblies Precision Replication on a mandrel 8” diameter corrugated mirror 50” radius of curvature mandrel Replicated to within 5 microns

Example: 60 nm RMS Lightweight Flat Mirror In 5 Days 9.55kg/m² Borosilicate (edge ring increased weight) Quality: 58 nm RMS / 310 nm P-V (@ 633nm)

Example: Precision Replication CO2 Interferogram Direct from Replication without Post-Processing Surface test of a replicated glass part molded to 2.3 waves (@ CO2 wavelength). Will meet CCAT finished specifications. CO2 CO2 interferogram Surface map

Corrugated Mirror Assemblies Alternative designs trade weight for stiffness 3,5, and 7 layer designs have been demonstrated in our process development project 3-Layers + Edge Ring 7-Layers with 3 Corrugations 5.76 kg/m² Demonstrated to 2” Deep 9.25kg/m² Sealed Core Design Demonstrated to 1.5” Deep

Corrugated Mirror Benefits Total process time per panel is short (~1 week) Benefit: High production rates, low cost per panel Areal densities below 10kg/m² have been demonstrated Benefit: Meets system requirements for overall weight Inexpensive raw material Benefit: Low cost per panel Several design approaches Benefit: Adequate trade space for design optimization Traditional mirror materials plus innovative manufacturing processes can meet the cost , schedule, and technical requirements of CCAT

Scale Up Risks Risk Mitigation We have successfully manufactured smaller demonstrator mirrors. Scaling to 2 meters is the predominate risk Risk Mitigation Large corrugation molds Segmented molds, ITT IR&D project Handling of large sheets Commercially available equipment Large scale precision slumping Evaluating process variables, ITT IR&D project Mold release over large areas Evaluating process variables,

Work to be Done with remaining CCAT funding Finish trade study for 3, 5, and 7 layer designs Select a prime approach Get formal quotes on material and delivery time ROM cost for panel fabrication Write report

Extra Slides Follow

Engineering Trade-Off A slightly smaller panel can be made thinner with less 1-G rms sag.

Error budget for panels

Layer Design 3 Layer Design (Core + 2 Plates) 50 mm deep 100 Hz first mode frequency Roughly 25 μm p-v gravity sag on optimized 3 point mount (including power) Roughly 10 μm p-v gravity sag on optimized 3 point mount (focusing out gravity induced power) 10 Kg/m2 Simpler, lower cost, more robust, lower performance

Layer Designs 5 Layer Design 200 mm deep design 300 Hz first mode frequency Roughly 2 μm p-v gravity sag on optimized 3 point mount (including power) Roughly 1 μm p-v gravity sag on optimized 3 point mount (focusing out gravity induced power) 8 Kg/m2 More expensive, more fragile, better performance