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Optical Perspectives Group

Optical Perspectives Group specializes in low-cost, easy to use and accurate instruments for aligning and centering optics and optical systems.

OPG was founded in 1992 to support optical fabrication and testing, and optical metrology instrument prototyping. The group evolved and since 2006 has focused on classical optical testing, optical assembly and alignment, particularly systems using aspheres.

Bob Parks of Optical Perspectives Group

Robert (Bob) Parks has broad experience to apply to your critical projects.

Curricula Vitae, Qualifications and Accomplishments

BA and MA in physics from Ohio Wesleyan University and Williams College


1967: Eastman Kodak Company; optical engineer

On his very first job assignment Bob had to use an autostigmatic microscope (ASM) to measure the radius of curvature of long radius test plates. At the time, he had no idea what he was using, how it worked, or that his whole career would be tied to variations of this test device.

Later, Bob and his office mate, Don Oinen, were the first people in the Research and Engineering Division to ask for, and get, a programmable calculator in their office so they did not have to submit all their simpler optical design calculations to the mainframe computer to get answers.


1969: Itek Corp.; optical test engineer

The six multi-color S-190 cameras for Space Lab were adjusted for magnification and focus by Bob and his technician Bob Sherlock. The 150 mm efl cameras with 70 mm film format had to be tuned so that the film from the cameras could be overlaid with less than +/- 2 micron image misalignment at the edges of the field even though the cameras operated in different spectral bands. This work was the genesis of the idea for attaching an electronic sensor, in this case a quad cell, in place of an eyepiece on an ASM because 2 of the cameras were used in the infrared and the light source was not visible to the eye.

Bob also started doing modal analysis of optical test wavefront errors by using Zernike polynomials to represent the wavefront errors. By quantitatively separating the wavefront errors into specific aberrations it made particular errors in the alignment of optical tests more obvious.


1972: Frank Cooke, Inc., Hands on optical fabrication experience

In order to better understand how to tolerance optical drawings Bob joined Frank Cooke at his optical shop in order to learn from a master how optics were made and learn of the tools available to the optician in working his or her craft. One thing that was immediately obvious at Cooke’s shop was that women were at least as good as men, if not better, as opticians.

One of the products Frank specialized in was hyper hemispheric glass domes. The inner and outer surfaces had to be concentric and the decenter had to be measured. Ray Boyd, the head metrologist, made a custom ASM by assembling a fiber preform that had been drawn into a small tip and bent down into the eyepiece of a microscope body. By shining a bright light on the exposed end of the preform, the microscope focused a bright spot at the centers of curvature of the surfaces of the dome. Spots reflected from the two surfaces were visible in the eyepiece and their separation laterally and in focus gave the decenter of the surfaces in 3 degrees of freedom. The simplicity of the technique and instrument made a lasting impression on Bob.


1976: Optical Sciences Center at the Univ. of Arizona; Optical Shop Manager

Through networking connections with Jim Wyant and Bob Fischer whom Bob knew from Itek, and the training he got at Frank Cooke’s shop, he was a perfect match for the opening at the College of Optical Sciences to manage the optical shop. One of his first tasks was to develop an algorithm to separate the errors in test optics from the errors in the mirror being tested by doing a rotational shear. This became the basis for further work by others in the area of absolute testing.

Another accomplishment was the specification and installation of a 6 m swing CNC precision grinder for contouring large aspheric mirror blanks. Even though the machine only had 32K of memory, Bob with the help of Bill Kuhn and Cary Kittrell, got the machine to do 3 dimensional contouring precise to the limits of the machine control.

The idea of an autostigmatic microscope (ASM) was advanced during this time making use of a commercially available eyepiece from EG&G with a fiber optic probe in the center of the field to act as the point source. The ASM proved a very useful optical test and alignment tool until the eyepiece went out of production and there was no replacement on the market.


1989: Optical fabrication and testing consulting, Allen Board of Investigation for the Hubble Telescope

Bob worked for the Allen Board of Investigation and spent extended periods at Hughes Danbury gathering background material for the Board. With the help of employees at Hughes Danbury, he located the apparent cause of the error, and helped write and edit the Allen Board report.

For his effort Bob received a NASA Public Service Medal in 1991.

These are color photos from the report.
End cap for measuring rod showing chipped paint around pinhole Fig 7-
Invar metering rod (B rod) with end cap in place and splice Fig 7-
Large test chamber with Hubble primary
RNC with test interferometer (CORI) on top
Reflective null corrector (RNC) with metering rod in position Fig 7-
Reverse null corrector

MORE INFO: The Hubble Space Telescope Optical Systems Failure Report


1992: Formed Optical Perspectives Group, LLC (OPG) with Bill Kuhn

One of the earlier consulting contracts that OPG got was from a local company, ETEC, building a laser scanner for printing PCB’s. The design included several toric lenses with rectangular outlines along with spherical lenses and mirrors whose centers of curvature had to be precisely aligned to the scanner’s optical axis. OPG built and patented (US Patent 6,924,897) an ASM that had an analog CCD camera and a Shack cube to produce a reference point for alignment.

The whole device was about 60x60x22 mm in size and easily attached to the ram of a coordinate measuring machine (CMM). Using the CMM as a large x-y-z stage it was easy to align all the optics to a common axis in a couple of hours rather than the weeks it had been taking using the touch probe on the CMM. Furthermore, the optical performance of the assembled lens was better than the prior assembly method.

Although the ASM worked well and the customer was very pleased with it, an obvious flaw was seen in the design. Once the reflected spot of light was overlapped with the reference spot the alignment could not be made better; one spot obscured the other. At the same time, Bill realized that with a digital camera and compatible software the reference spot could be created electronically and the reflected spot made to coincide with the reference to less than a micron by centroiding on the reflected spot. This was the basis of what is now sold as the PSM, the design of which was almost all Bill’s.

The first couple of PSM’s were purchased by the Breault Research Organization for the alignment of an off-axis two mirror telescope and by Raytheon Missiles Systems by an engineer who had worked at ETEC and realized how the PSM would aid in the alignment of some of the optics at Raytheon.

Further ideas of how the PSM can be used for alignment and test are shown in the Technical Library section of the web site, in PSM Application Notes.

Key Contributions:

US representative to the ISO Technical Committee 172 on Optics and Optical Instruments

Chairman of the ISO Subcommittee 1 for Fundamental Optical Standards

SPIE: Fellow and past member board of directors

American Society for Precision Engineering, President & Lifetime Achievement Award

Optical Society of America, member

U.S. Patents:

  • Method and apparatus for absolute optical measurement of entire surfaces of flats 5,502,566
  • Rapidly renewable polishing lap 5,897,424
  • Dual beam spectrophotometer modular sample system 6,870,615
  • Point source module and methods of aligning and using the same 6,924,897
  • System and Method for Non-Contact Metrology of Surfaces 9,068,904

 

The Point Source Microscope (PSM) and CaliBall emerged from customer projects. The pursuit of optimal system performance required new tools to make alignment and component manufacturing easier. OPG now offers the PSM and CaliBall as products as well as the MicroFinish Topographer (MFT)and Centering Stations.

Point Source Microscope

Point Source Microscope

PSM Point Source Microscope

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MicroFinish Topographer

MicroFinish Topographer

Universal Surface Roughness Measurement

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Centering Station for PSM

Centering Station for PSM

Centering Station for PSM Point Source Microscope

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CaliBall I & II

CaliBall I & II

CaliBall, a calibration artifact using the Random Ball Test

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