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A Contemporary Version of the Autostigmatic Microscope and Its Uses

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  • OUTLINE

    What is an autostigmatic microscope (ASM)
  • Measuring the radius of curvature of a concave surface
    – Main historical use
  • Modern version of an ASM uses internal infinite conjugate optics
  • Use of an ASM for alignment of optical systems
  • Other uses of an ASM
  • Conclusions
 

Description of an ASM

  • First description in English literature is Drysdale, Trans. Opt. Soc. London, 1900


  • Fig. 2 from the Drysdale paper of 1900


  • Further from the Drysdale paper


Cat’s eye and confocal foci

Cat’s eye

Cat’s eye

Cat’s eye reflection

  • Objective focused on surface
  • Out going rays re-enter on opposite side of objective
  • If surface tilted, reflected rays parallel outgoing rays in collimated space
  • Cat’s eye used for setting crosshairs
  • Cat’s eye used for setting reference

Confocal foci

Confocal foci

Confocal reflection

  • Rays focused at center of curvature
  • Rays hit surface at near normal incidence and re-trace themselves
  • If surface tilted, rays do not re-trace and will not center on crosshairs
  • Confocal used for alignment
  • Confocal for bringing CofC to reference


Examples of Cat’s eye and CofC spot images

Out of focus Cat’s eye spot image

Out of focus Cat’s eye spot image

In focus Cat’s eye

In focus Cat’s eye

Notice Shutter and Gain with focus

Locating an ephemeral point in space with 3 degrees of freedom to μm precision

 
Out of focus & decentered CofC spot

Out of focus & decentered CofC spot

In focus but decentered CofC spot

In focus but decentered CofC spot

In focus and centered CofC spot

In focus and centered CofC spot



Measurement of radius of curvature

Consists of three steps:

  1. Focus on the concave mirror surface to get a Cat’s eye reflection
    Set the reticle or electronic cross hairs on the reflected point image
    This established the optical axis of the ASM

  2. Move the ASM back to near the center of curvature of the concave mirror
    Locate the reflected focused spot which may not be aligned to the objective
    Tilt the mirror until the reflected focused spot enters the objective
    Focus the ASM on the reflected spot and center it on the crosshairs
    Note the distance of the ASM on a linear scale

  3. Move the ASM forward until it is focused on the mirror surface
    Moving from center of curvature means moving on a normal to the surface
    Get a sharp focus the Cat’s eye reflection
    Cat’s eye reflection will necessarily be centered on the cross hairs
    Read the distance of the ASM on the linear scale
    The difference of the Cat’s eye and confocal positions is the radius of curvature of the mirror


Measurement of radius of curvature

 

    1. Focus on surface, used Cat’s eye reflection to set crosshairs
    2. Move to confocal, adjust microscope so reflected spot in focus and centered on crosshairs, note linear scale reading
    3. Move to focus on surface and get well focused Cat’s eye spot. Note scale reading
      Difference in readings is the radius of curvature



If this concept is well understood all other applications are easy




Measurement of long radius of curvature
Use defocused collimator

    1. Find s by putting a plane mirror in front of collimator
    2. Put long radius surface in front of collimator and note ds
    3. Since to first order efl = s, 1/s = 1/(s – ds) + 1/R, we find R = -s(1 + (s/ds))
      (Be careful of signs, use common sense)


A contemporary version of the ASM
 is three instruments in one

  • Autostigmatic microscope
  • Internal SM fiber source
  • Electronic autocollimator
  • Simply remove objective
  • Video imaging microscope
  • Image plane parafocal with ASM focus
  • Internal LED Kohler source


Some advantages of the contemporary design

Use of solid state light sources – compact, internal, low heat, monochromatic
SM fiber coupled laser diode – bright for ease of alignment, near perfect spot
Video camera – ergonomic, high position sensitivity, settable reference
Software – permits high resolution centroiding on reflected spot
  • Large dynamic range on reflected light intensities
  • Recording and storage of Star images for optical quality determination
  • Centroid data easily coupled into other scales, a CMM, for example


Other uses of the ASM; designed for alignment

Perfect for locating centers of curvature and foci of optical systems
Use as a sensor on a centering station using a rotary table to define an axis

Use was to align the elements of a f-theta laser scanner lens to a common axis
Lens system had spherical and toroidal lenses and an “off-axis” mirror
ASM mounted to the ram of a coordinate measuring machine
Used a large x, y, z stage to pick up centers of curvature and align to axis
  • Don’t think like a lens designer and where rays go
  • Think about where centers of curvature should go and how to get them on a common axis


Use two ASM’s to align an “off-axis” lens

Radius of convex side longer than working distance of objective, need extra lens


Set-up using 2 ASM’s to align lens



Alignment of fold mirrors

Plane fold mirrors have 3 degrees of freedom, 2 tilt and one displacement<
Optical and mechanical design will show where the center of curvature should be located when the fold mirror is proper aligned
A ball in a fixture will mechanically locate this position, and ASM can verify


Another example of a fixture for alignment



The role of steel balls in alignment

Steel balls are a physical realization of a point in space
Something you can physically touch as opposed to a theoretical object
The ball center, the “point”, defines 3 translational degrees of freedom in space
The ASM transfers an optical point, a CofC or focus, something you cannot touch, to the center of a ball, something that can be located physically
Steel balls are inexpensive, extremely precise and come in many sizes
Grade 5 chrome steel balls are round to 125 nm and cost about $3 each
Can be thought of as convex optical grade mirrors
Plug gauges are the cylindrical equivalent of balls and define axes in 3 DofF
(Plug gauges are Go/no go pins for gauging the size of holes)


Alignment using aberrations

An ASM is a “Star” test device showing the point spread of an aberrated wavefront
It has sensitivity to about lambda/8 or lambda/10
Useful for quick check of quality of optical surfaces as they are assembled into systems
Alignment of a parabola as an example
Initially the return spot will not be centered on the crosshairs of the ASM
The parabola or autocollimating mirror are tilted until return spot on crosshairs


Alignment using aberrations (con't)

When return spot lies on the crosshairs, the rays strike the flat at normal incidence
However, the normal to the flat may not be parallel to axis of parabola
As a consequence, the return spot will show coma
To finish the alignment, tilt the flat while keeping return spot on the crosshairs until the coma is reduced to a symmetrical spot.
The entire alignment process takes only minutes to accomplish


Other uses of an ASM – Finding lens conjugates



Finding first order lens conjugates

Finding the radius of curvature of one side is direct measurement
This assumes it is concave or there is sufficient working distance

Almost any lens can be reversed and measured through the side if not enough working distance

To find the other conjugates it is necessary to model with a lens design program
Or use first order equations and an iterative equation solving program
See Parks, R. E., “Measuring the four paraxial…, Appl. Opts., 54, 9284 (2015)


Zero index material – a useful trick

When using an ASM or an interferometer most setups are double pass
Light comes from the instrument, reflects at normal incidence off the last surface and retraces itself back into the instrument
For a quick insight to the test it is a lot of work to trace a double pass system
The trick; reverse the system and make rays leave the last surface at normal incidence
To do this have rays from infinity travel through a medium of 0 index to the last surface
Then n*sin(θ) = n’*sin(θ’) = 0, so θ’ = 0, or the rays leave the last surface normal to it!
Now a marginal ray height solve after the last refraction shows the paraxial focus
Credit for the idea; I don’t know who deserves it
I learned it from Jim Burge at UofA, Optical Sciences
I suspect he may have learned it from Roland Shack
If someone knows a better attribution I like to know.


An example – finding CofC’s and surfaces

Assume a simple optical system such as an air spaced doublet
Find the centers of curvature and surfaces vertices looking into the system
Reverse elements, object at infinity and n = 0, float by stop on last surface
MRH = 26.403     = 24.395     = 39.445     = -94.453
Object on first surface, image space f/# large, stop on last surface
MRH = -7.471      = -5.492      = -3.368      = 0


Find the index of refraction of a ball

For small angles a = h/2r, and the normal = 2a, so the refracted ray angle is an/2
The ray angle relative to the x axis is 2a – an/2 = a(1-n/2)
The mrh = h/(h/r(1-n/2)) = 2r/(2-n)
Or, n = 2(mrh – r)/mrh
Works even if ball behind a window in a thermal chamber, but use ray trace


Find the index of a liquid and radius of a submerged surface



Measurement of angle

As shown earlier, by simply removing the objective the ASM is an autocollimator with sub-arc second sensitivity
The bright mode of the laser source makes initial alignment easy in ambient light
The small beam size makes it particularly useful for inspecting small prisms


ASM’s and computer generated holograms

A CGH pattern can simulate a ball, that is focus light a specific distance above the CGH

If balls are used to kinematically locate a CGH, a pattern to locate the balls can be included as part of the overall pattern. Then an ASM can precisely locate the balls. The balls, cemented in place, become an integral part of the CGH test artifact.

Because a CGH pattern can simulate a ball, a CGH can be made as an artifact for locating a group of points in space precisely located to < 1 μm in 3 dimensions.

An ASM mounted on a robot arm, for example, could be used to pick up the points one at a time to train and calibrate the robot.



Example of CGH hologram

Printed on a 150 mm square photomask substrate
Each circular pattern produces points several distances above the CGH
Actual photograph is not available at the moment
CGH courtesy of Arizona Optical Metrology, LLC, www.cghnulls.com


Conclusions

While autostigmatic microscopes (ASM) are over 100 years old, modern technology makes them truly practical for many diverse optical metrology needs.


Once the basic operation of measuring the radius of curvature with an ASM is understood, it becomes obvious that an ASM has many more useful applications.


Almost everything discussed here can also be done with an interferometer with greater precision. However, if the ultimate in precision is not needed the ASM is more convenient to use because of its small size, light weight and ease of mounting. Further, in some applications the greater coherence of an interferometer make some of the applications more difficult to perform because of multiple fringe patterns.


In many instances an ASM is a cost effective and easy to use alternative to an interferometer.

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About the Author

Robert Parks

Robert Parks

Robert Parks received a BA and MA in physics from Ohio Wesleyan University and Williams College, respectively. His career started at Eastman Kodak Company as an optical engineer and then went on to Itek Corp. as an optical test engineer.

He learned about optical fabrication during a 4 year stay at Frank Cooke, Inc. This experience led to a position as manager of the optics shop at the College of Optical Sciences at the Univ. of Arizona and where he worked for 12 years and had a title of Assistant Research Professor. During that time he had the opportunity to write about the projects in the shop and the optical fabrication and testing techniques used there including papers about absolute testing and the installation and used of a 5 m swing precision optical generator.

Mr. Parks left the University in 1989 to start a consulting business specializing in optical fabrication and testing. Among the consulting projects was one working for the Allen Board of Investigation for the Hubble Telescope where he stayed in residence at HDOS for the duration of the investigation. In 1992 he formed Optical Perspectives Group, LLC as a partnership with Bill Kuhn, then a PhD student at Optical Sciences.

The consulting and experience with Optical Perspectives provided many more opportunities to publish work on optical test methods and applications. While still at Optical Sciences, Mr. Parks became involved in standards work and for twenty years was one of the US representatives to the ISO Technical Committee 172 on Optics and Optical Instruments. For two years he was the Chairman of the ISO Subcommittee 1 for Fundamental Optical standards. Recently Mr. Parks temporarily rejoined Optical Sciences part time helping support optical fabrication projects and teaching as part of the Opto-Mechanics program.

Bob is a member of the Optical Society of America, a Fellow and past Board member of SPIE and a member and past President of the American Society for Precision Engineering. He is author or co-author of well over 100 papers and articles about optical fabrication and testing, and co-inventor on 6 US patents. He remains active in development of new methods of optical testing and alignment.

Case Studies & Testimonials

  • Sometimes good news goes unnoticed for the longest time. We just stumbled on this unattributed, but complimentary note about the PSM.
    See  https://www.idex-hs.com/wp-content/uploads/2018/05/Enabling-Micron-Level-Mounting-Accuracy.pdf   

    Notice the PSM in the top center of Fig. 9.  Thank you, IDEX.

  • "We are enjoying our Point Source Microscope and finding it invaluable in alignment and diagnostic tasks."

    Dr. John Mitchell
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  • "Just wanted to share a recent success aligning an adaptive optics test bed with the PSM. We used to use a traditional alignment telescope in the past, but the PSM made the whole process really easy and fast. The main requirements were to quickly determine the quality of beam collimation and pupil conjugates since there are several beam expanders and compressors with multiple pupil and focal planes."

    Suresh Sivanandam
    Dunlap Institute for Astronomy and Astrophysics
    University of Toronto

     

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    Hart Scientific Consulting International, LLC
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