The use of slope specifications for optical components

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Jim Burge College of Optical Sciences University of Arizona Tucson, AZ 85721 [email protected] The use of slope specifications for optical components Presented at: 2010 APOMA Workshop (American Precision Optics Manufacturers Association) Tucson, Arizona, November 10, 11 (2010)

Transcript of The use of slope specifications for optical components

Page 1: The use of slope specifications for optical components

Jim Burge

College of Optical SciencesUniversity of ArizonaTucson, AZ 85721

[email protected]

The use of slope specifications for optical components

Presented at:

2010 APOMA Workshop (American Precision Optics Manufacturers Association)Tucson, Arizona, November 10, 11 (2010)

Page 2: The use of slope specifications for optical components

Wavefront error vs Image shape

x i n

y i n

W B FxW B Fy

ε

ε

∂= − ⋅

∂∂

= − ⋅∂

For each ray:εx, εy are errors in ray position at focal plane

Wi is wavefront error from surface i

are wavefront slope errors (dimensionless)

Bi is diameter of beam footprint from single field point(< diameter of the element)

FN is system focal ratio

yW

xW

∂∂

⋅∂∂ ,

εy

εx

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Wavefront – Gradient – Image degradation

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Image blur due to errors in element 1: Blur rms = refers to rms slope variation over the footprint

Image distortion due to errors in element 1:refers to the average slope over a footprint

Geometry definition

( ) 1rms nrmsW B Fε = ∇ ⋅ ( ) 1rms nrms

W B Fε = ∇ ⋅

( ) 1 nmeanW B Fε = ∇ ⋅vv

B1

12nF

NA=

( )mean

W∇v

( ) 1rms nrmsW B Fε = ∇ ⋅

( )rmsW∇

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Surface irregularityFor 1 µm P-V surface irregularity:

Surface Error RMS surface error ΔS (µm)

Normalized RMS surface slope (µm/radius)

Focus 0.29 1.43 Astigmatism 0.20 0.72

Coma 0.18 1.24 4th order spherical aberration 0.30 3.35

Trefoil 0.18 0.89 4th order astigmatism 0.16 1.58

5th order coma 0.14 2.04 6th order spherical aberration 0.19 3.50

Sinusoidal ripples, frequency of N cycles across the diameter

0.35 1.11 N

Rule of thumb for small spherical optics 0.25 2

Normalized to 1 µm PV. Scale to get ΔS and Θs

Normalized slopes given in µm/radius where the radius = half of the diameter.

To get slopes in µradians, divide normalized slope (in µm/radius) by the radius (half-diameter) of the part in meters

1 for < 2” optics2 for > 6” optics

Rules of Thumb

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Standard Operating Procedure• Most optical systems are not diffraction limited.

– Wavefront errors are > 1 λ, image size is bigger than λFn

– System performance can be quantified with spot size, encircled energy, MTF, etc. based on geometric (ray trace) analysis.

• For the case where the system is not diffraction limited, image blur is proportional to errors in ray angle, which can be caused by slope variations- the geometric limit

• Most optical surfaces are qualified based on the error in the surface profile– Resulting wavefront error is proportional to surface error

• Scale factor depends on refractive index or mirror

– The resulting slope errors depend on the form of the error– To estimate system performance from profile error, you have to know (or

assume) the form of the profile error.

The surface profile specification is not directly related to system performance, which frequently causes:1. Designers over-specify components to insure performance2. Systems may not meet requirements, even though the components are in spec.

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Slope specifications for surfaces and elements

• The problems above are avoided by specifying errors in terms of slope, or the first derivative of the surface profile

Slope can be quantified using µrad, nm/cm, waves/inch,…

• Advantages:– Slope measurements are easier and lower cost than transmitted

wavefront measurements– Slope errors can be directly scaled to provide effect on image

quality or distortion• Disadvantages

– Must define band limit. Once frequencies become high, the slopes for insignificant ripples and noise become meaningless. A natural band limit can be defined by diffraction.

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Effect of surface irregularity, rms spot size

( )rms i nrmsW B Fε = ∇

( ) ( 1)cos( )rmsrmsW n φ∇ ≈ Θ × −

( 1)cos( )rms rms i nn B Fε φ= Θ − ⋅

1. Convert the normalized surface slope Θ to wavefront slope

2. Relate rms wavefront slope to rms spot size (via Optical Invariant)Bi = beam footprint diameter from single field pointFn is system working focal ratio

W∇

RMS Surface slope (radians)

Convert to wavefront using refractive index, angle of incidence (for mirror, n = -1)

Measure transmitted wavefront slope directly, then scale to get contribution to image blur

Or determine transmitted wavefront slope from surface slope

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System error budget• Total contribution from each element taken as RSS

( ) ( )( )2 2 2 2

2 22 2 2 21 1 2 2

...

...

total design alignment surfaces

surfaces nF B W B W

ε ε ε ε

ε

= + + +

= ⋅ ⋅ ∇ + ⋅ ∇ +

B1 B5

12nF

NA=

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Orthonormal basis for slope errors• Zernike polynomials are used to represent surface shape of wavefront• We developed Zernike slope polynomials to represent vector functions

• These are orthonormal: ∑=∂

∂+

∂∂ ),(ˆˆ yxSaj

yWi

xW

ii

r

C. Zhao and J. H. Burge, “Orthonormal vector polynomials in a unit circle, Part I: basis set derived from gradients of Zernike polynomials,”Optics Express 15, 18014‐18024 (2007).

∑= 2irms aslope

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Measurement

• Slope error can be measured directly for surfaces, components, and systems

• Slope measurements are generally much easier than profile or wavefront. (insensitive to phase shift)

• SCOTS (Software Configurable Optical Test System) provides low cost method of performing such measurements over a very wide dynamic range with sub-µrad accuracy.

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Vision for the future

• Optical components could be specified with tolerances on prescription (R, n, t) and transmitted slope errors

• Error analysis is easy because slope errors directly relate to image degradation – no additional MSF spec

• Determine slope variation in final parts– Use interferometry if you want, then process the data to

determine slope– Better yet, acceptance testing could be done with simple SCOTS

type system. Uncertainties in the test will be quantified in terms of slope.

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Implementation

• Implement low cost slope measurement system (SCOTS)

• Perform systematic sampling of optical elements to establish some database on the statistics of slope errors from your manufacturing process.

• Offer elements according to class of slope errors, ie.– Grade 1 < 1 µrad rms– Grade 2 < 5 µrad– Grade 3 < 25 µradUnspecified < 100 µrad

• Test of each lens is quick, and can be automated.

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Outcome

At the systems level• Avoid over-specification • Insure that systems will meet requirements, based on

analysis and component testing.

For the manufacturer• Offer low-cost, quantitative testing of each element,

providing meaningful quantity• Potentially feedback to the processing to provide higher

performance parts, higher yield, or lower manufacturing costs optimizing the quantity that really drives performance – the slope.