Optical Fabrication and Testing

Optical Fabrication and Testing

09 - 13 July 2017
Denver Marriott City Center, Denver, Colorado United States

OF&T, will offer new ideas and concepts for the shaping, smoothing, testing and manufacture of conventional and novel optics/optical systems finding applications in existing and emerging technologies.
 
The 2017 Optical Fabrication and Testing Topical Meeting (OF&T) will emphasize new ideas, concepts and emerging applications in optics manufacturing and metrology. Hot topics will include the following: fabrication of optics by lasers, additive manufacturing of optical components, molding of micro-optics, deterministic manufacturing of aspheric/conformal/freeform optics, advanced metrology systems and direct slope/curvature measurement, fabrication of optics from novel materials, efficient manufacturing and testing of large optics, new CNC machining processes and advances in finishing science. Papers that describe manufacturing chains from the generation of complex shapes to the fine finishing of surfaces, giving details of the process science, will be especially welcomed.


1. Optical Materials
  • New materials for new applications (composites, plastics, crystals, glasses, lightweight materials, ceramics, carbides, chalcogenides, UV optical materials, additive manufacturing)
  • Material properties and the response to fabrication processes
2. Grinding and Polishing
  • Grinding, precision grinding, diamond turning and milling, ultrasound assisted machining, vibration assisted polishing, processing of edges
  • New ideas in traditional (pitch) polishing, magnetic field-assisted finishing, ion beam figuring and polishing, fluid-jet polishing, novel finishing processes
  • Abrasives, novel abrasive formulations, abrasive-impregnated pads
3. Figuring and Finishing Science (Laser Processing, etc.)
  • Fabrication or polishing of optics with lasers or concentrated light
  • Tailored slurries through the adjustment of pH and zeta potential
  • Deterministic figuring techniques, mid-to-high spatial frequency error control, and various smoothing approaches during computer controlled optical surfacing
4. Optical Testing and Advanced Metrology Systems
  • Testing for sub-surface damage, homogeneity, form, finish and scratch/dig
  • Measurement, interpretation, and applications of power spectral density
  • New ideas in interferometry, direct slope/curvature measurement
  • Testing aspheric surfaces with and without null-optics, reconfigurable nulls
  • Computer-generated holograms and spatial light modulators for testing
  • Absolute tests for flats, spheres and aspheres
  • New concepts in profilometry: optical and mechanical probes
  • Testing of very small optics
  • White light interferometry, fringe projection metrology, deflectometry
  • Testing in adverse environments: vibration, turbulence, vacuum, and space
  • In-process metrology
  • Testing of freeform surfaces
5. Assembly, Alignment, Contamination Control, Cleaning, Packaging
  • Adhesives and cements for elevated, ambient and low temperature
  • Stable joining of optical surfaces by optical contacting, direct bonding or laser welding
  • Alignment of optical components and systems containing aspheric elements
  • Alignment of multi-element mirrors
  • Measurement and control of deformation and stress birefringence in mounting
  • Cleaning optics, clean rooms and contamination control
  • Handling and packaging of precision optics
6. Process Engineering
  • Glass and plastic (micro) molding to high surface accuracy and low surface roughness
  • Cost effective optics manufacturing processes
  • Engineering gradient index optics
  • Cost effective fabrication of aspheric surfaces
  • Automation of the manufacturing chain in optics fabrication
  • Good and bad experiences from the shop floor
7. Fabricating Next Generation Optical Systems (Freeform Optics, etc.)
  • Photolithography optics
  • Adaptive optics
  • Integrated optics
  • Freeform optical systems and industrial manufacturing
8. Large Optics
  • Fabrication and testing of large optics for EUV and x-ray applications
  • Large optics for earth-based and space-based astronomy
9. Nanostructures and Films
  • Characterization of coatings for advanced laser optics
  • Nanostructures on optical surfaces
10. Education and Training in Optics Metrology and Finishing Science
  • Uncertainty and traceability
  • Interpretation of metrics for optical surface characterization
Andreas Beutler, Mahr GmbHGermany
Referencing and Form Measurements of Freeform Optics, Invited

Glen Cole, Thirty Meter TelescopeUnited States
Optical Fabrication and Metrology for the Thirty Meter Telescope Primary Mirror Segments, Invited

Turan Erdogan, Plymouth Grating Laboratory, Inc.United States
Manufacturing Large-format Spherical and Cylindrical Laser Focusing Gratings using Scanning-beam Interference Lithography, Invited

Oliver Faehnle, FISBA OPTIK AGSwitzerland
Machine Acceleration Effects on Computer Controlled Polishing, Invited

James Fienup, University of RochesterUnited States
Phase Retrieval for Optical Metrology: Past, Present and Future, Invited

Mohammadreza Khorasaninejad, University of WaterlooUnited States
Optics with Metasurfaces: Beyond Refractive and Diffractive Optics, Invited

Manyalibo Matthews, Lawrence Livermore National LaboratoryUnited States
IR Laser Processing Techniques for NIF Optics, Invited

Cormic Merle, United States
Metrology for the LSST M2: Large Holographic Stitching Technique, Invited

Brigid Mullany, Univ of North Carolina at CharlotteUnited States
Fiber Based Polishing Tools for Optical Applications, Invited

Mahito Negishi, Canon IncJapan
New Stitching Algorithm using an Approximated Reference Shape, Invited

Joseph Owen, Univ of North Carolina at Charlotte
Diamond Milling of IR Materials, Invited

Jyrki Saarinen, HeptagonFinland
Additive Manufacturing for Small and Medium Sized Optics, Invited

John Schaefer, ELCAN Optical TechnologiesUnited States
Advances in Diamond Turning, Invited

Sven Schröder, Fraunhofer IOFGermany
Surface Characterization of High-End Optical Components using Light Scattering, Invited

Robert Smythe, Apre InstrumentsUnited States
Interferometric Measurement of Mid-Spatial Frequency Wavefront Errors, Invited

Simon Thiele, University of Stuttgart, ITOGermany
Complex Micro-optics by Femtosecond Direct Laser Writing, Invited

Jurgen Van Erps, Vrije Universiteit BrusselBelgium
Prototyping and Replication of Polymer Freeform Optical Components, Invited

Reinhard Voelkel, SUSS MicroOptics SASwitzerland
Novel Fabrication and Testing Methods for Micro Optics, Invited

Christian Weingarten, Fraunhofer ILT
Combination of Laser-based Process Steps for Optics Manufacturing, Invited

Richard Youngworth, Light Capture, Inc.United States
Adopting and Using Optical Standards, Invited

Chairs

Jessica DeGroote Nelson, Optimax Systems Inc., USA Matthew Jenkins, Raytheon Company, USA
Dae Wook Kim, University of Arizona, USA

Members

Dave Aikens, Savvy Optics Corp, USA Andreas Beutler, Mahr GmbH, Germany Myung Cho, AURA NOAO, USA
Tolis Deslis, JENOPTIK Optical Systems, LLC, USA Jonathan Ellis, University of Rochester, USA
Chris Evans, Univ of North Carolina at Charlotte, USA Oliver Faehnle, FISBA OPTIK AG, Switzerland
Eric Fest, University of Arizona, USA
Kyle Fuerschbach, Sandia National Laboratories, USA
Ulf Griesmann, National Inst. of Standards & Technology, USA Sven Kiontke, Asphericon GmbH, Germany
James Mooney, Harris, USA
Soojong Pak, Kyung Hee University, South Korea Michael Ponting, PolymerPlus LLC, USA
Christof Pruss, Universität Stuttgart, Germany Jannick Rolland, University of Rochester, USA Sven Schröder, Fraunhofer IOF, Germany Katie Schwertz, Edmund Optics, USA
Tayyab Suratwala, Lawrence Livermore National Laboratory, USA Hideo Takino, Chiba Institute of Technology, Japan
Flemming Tinker, Aperture Optical Sciences, USA Ray Williamson, Ray Williamson Consulting, USA

Congress Special Events

Short Course - Meaningful Scratch and Dig Specifications
9 July, 14:00-18:00

Dave Aikens, the Presider and found of Savvy Optics Corp. will present this course. Visit the Short Course page for complete information. There is an adidtional cost for attending the course and includes a copy of the notes.  

Opening Plenary Session
10 July, 8:00-10:00
  • Patrick McCarthy Giant Magellan Telescope, USA
  • Joshua Smith California State University Fullerton, USA
  • Jannick Rolland University of Rochester, USA
Visit the plenary page for complete information on each speaker and their talk. 

Closing the Wage Gap - AAUW Work Smart Salary Negotiation
10 July, 12:30 – 14:00

Join us for an interactive workshop focused on closing the wage gap and providing attendees resources designed to help negotiate for a new job, raise, or promotion. Attendees will gain confidence in negotiation style through facilitated discussion and role-play.
  • How to identify and articulate your personal value
  • How to develop an arsenal of persuasive responses and other negotiation strategies, including how to get a raise or promotion
  • How to conduct objective market research to benchmark a target salary and benefits
  • About the wage gap, including its long-term consequences
Why is negotiation so important? AAUW’s research on the gender pay gap shows that, one year out of college, women are already paid significantly less than their male counterparts. Women who work full time take home 80 cents for every dollar a full-time male worker is paid. And over a lifetime, those lost potential earnings add up.

Workshops are open to OSA Members. Space is limited and we ask that you RSVP online.
 
Hosted by:
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Congress Barb-B-Q
10 July, 18:00-20:00

Join your fellow attendees for a Western Style Barb-B-Q. Enjoy delectable fare while networking. The BBQ is open to committee/presenting author/student and full conference attendees. Conference attendees may purchase extra tickets for their guest. 

Creating Effective Conference Posters Lunch & Learn
11 July, 12:30 – 14:00

Join us for an interactive lunch & learn program focused on creating effective conference posters. Jean-luc Dumont will provide relevant examples and real life experiences to enhance your communication and conference poster development. You will leave this workshop with an understand of the best practices in poster creation and presentation. Lunch will be provided.

This program is open to OSA Members. Space is limited and we ask that you RSVP online.
 
Hosted by:


Joint Poster Session
11 July, 18:00-19:30

Posters are an integral part of the technical program and offer a unique networking opportunity, where presenters can discuss their results one-to-one with interested parties. Each author is provided with a board on which to display the summary and results of his or her paper. 

IODC Illumination and Lens Design Problems Presentation
12 July, 18:00-20:00

Join the IODC community for a guaranteed highlight of the conference: the illumination and lens design contest presentations. As usual, significant work has gone into developing and scoring the submissions, as well as all of the hard work put in by solution submitters. Vist the contest page for complete information. 

Plenary Speakers

Patrick McCarthy
Giant Magellan Telescope, USA

Giant Magellan Telescope, Optics and Science





The world’s next great astronomical observatory – The Giant Magellan Telescope – will be used to explore the early Universe and to search for life on other planets. I will describe the scientific mission and the engineering challenges involved in its design and construction.



Bio: Patrick McCarthy is the Interim President of the Giant Magellan Telescope Project. He received his Ph. D., in Astronomy from U. C. Berkeley in 1988. He went to the Carnegie Observatories first as a Carnegie Fellow and then as a Hubble Fellow in 1991. In 1993 he joined the scientific staff at Carnegie. He is known for his work on galaxies in the distant universe and, in particular, for his study of distant low frequency cosmic radio sources: sign posts to massive galaxies undergoing rapid accretion on to super massive black holes. In the late 1990s, McCarthy and his colleagues identified a new population of galaxies with colors indicative of very early star formation. Study of these faint red galaxies is now one of the most active areas of research in astrophysics.
 
McCarthy has been active in scientific and management oversight of large science projects and organizations. He has chaired numerous panels for NASA and the NSF providing independent oversight of the Hubble Space, Spitzer Space Telescope, and large telescopes on the ground. McCarthy led the Giant Magellan Telescope (GMT) Science Working Group that wrote the scientific case for the telescope project and defined the scientific and technical requirements for the facility.
 
Today, he leads the team of scientists and engineers building the Giant Magellan Telescope (GMT), an enormous instrument comprised of seven primary mirror segments—the seven largest mirrors ever made—that will stretch to more than 80 feet across once complete. The GMT will explore the cosmos to observe the first stars in the universe, offering images 10 times sharper than those coming from the Hubble Space Telescope. Since 2008, he has served as the head of the non-profit corporation, GMTO, that is charged with carrying out the development, construction and operation of the telescope and related facilities. My day-to-day responsibilities include ensuring that the telescope and its instruments will be able to address the key questions at the forefront of astrophysics in 2020 and beyond.

Joshua Smith
California State University Fullerton, USA

Using Optics and Precision Metrology in to Measure Black Hole Mergers from Across the Universe with LIGO

On September 14, 2015 the two detectors of the Laser Interferometer Gravitational Wave Observatory (LIGO) detected gravitational waves from the merger of a binary system of black holes. This discovery could not have been made without a century of advances in optical technology and precision metrology. I will give an overview of gravitational waves detected by LIGO to date and describe the optics involved and current optical challenges. I will end with prospects for future gravitational-wave observations made with even more advanced optics.


Bio: Joshua Smith directs the Gravitational-Wave Physics and Astronomy Center (GWPAC) and is an associate professor of physics at California State University, Fullerton. Currently he is active in gravitational research, astronomy education research, and teaching physics and astronomy. His research is focused on detecting gravitational waves from astronomical sources using the Laser Interferometer Gravitational-wave Observatory (LIGO) in collaboration with colleagues in GWPAC and in the international LIGO Scientific Collaboration. 

Jannick Rolland
University of Rochester, USA

Freeform Optics from Design to Manufacture and its Envisioned Impact on Technology to Enable the Science of Tomorrow


All-reflective optical solutions have long hold their place in optical system design from small scale optics as in microscopes to large scale optics as in telescopes. Yet reflective solutions have suffered from obscuration or the need to restrain surfaces to be off-axis conics or aspherics. The ability to recently fabricate freeform surfaces opens up new spaces for optical design, driven by applications spanning demands in mobility, larger fields of view, apertures, light weight and compactness.  I will present success stories designing and prototyping designs with freeform surfaces and highlight pathways and challenges associated with their emergence.

Bio: Jannick Rolland is the Brian J. Thompson Professor of Optical Engineering at the University of Rochester and she directs the NSF I/UCRC Center for Freeform Optics (CeFO).
 
Rolland joined the University of Rochester in 2009 after advancing her career from Assistant to Full Professor at CREOL, the College of Optics and Photonics at the University of Central Florida.  Together with colleagues at the University of Rochester and partners at the University of North Carolina at Charlotte, she launched in 2013 the Center for Freeform Optics (CeFO) as an international consortium aimed at advancing the science and engineering of freeform optics.  Rolland earned an optical engineering diploma from the Institut D'Optique Théorique et Appliquée, France, and a PhD in Optical Science from the College of Optical Sciences at the University of Arizona. She is a Fellow of OSA, SPIE, and NYSTAR. She is the recipient of the 2014 OSA David Richardson Medal. She is known for her innovations since the 90s in head-worn displays, and more recently her innovations in 3D microscopy and telescope designs.