Mach-Zehnder Interferometer for 2-D GRIN Profile Measurement

 
Mach-Zehnder Interferometer for
2-D GRIN Profile Measurement
 
Instrument Overview
Sample Preparation
Measurement Uncertainty
 
University of Rochester
Gradient-Index Research Group
 
2D GRIN Measurement: Mach-Zehnder Interferometer
 
Wavelength range covered
0.355 – 1.064
μ
m, 1.55 – 4.6
μ
m, 8 – 12
μ
m
Measurement accuracy
δ(
Δ
n) = 1E-5
Beam size: 65mm x 40mm ellipse
Sample prep requirements
Thin (~1mm), plane, parallel sample with GRIN
“exposed” (index is constant through sample
thickness)
 
Measure: 
, t
Calculate: 
Δ
n
Laser
 
Spatial
Filter
 
Beam
Splitter
 
Beam
Splitter
 
Mirror
 
Mirror
 
Sample
 
Lens
 
Detector
 
GRIN Blank
 
Measurement
Slice
 
Measured
Interferogram
 
2
 
Mach-Zehnder Sample Prep
 
GRIN Blank
 
Measurement
Slice
 
Measured
Interferogram
 
Radial
 
Axial
 
Sample thickness chosen so
that # of fringes can be
resolved by imaging optics
and detector
Surface figure error and
wedge lead to
measurement error
 
Thin slice cross-section that “exposes” the
gradient for measurement
Index should be constant through the thickness of
the sample (z-axis)
 
x
 
y
 
3
 
Mach-Zehnder Measurement Uncertainty
 
Best-case uncertainty is
determined by a root-sum-square
of the terms in the 
Δ
n calculation
 
m
 = # of fringes
λ
 = wavelength
t
 = thickness
 
Uncertainty is increased further by surface figure error and wedge, but it can be
minimized by measuring in an index matching fluid
 
Use the calculator on the next slide to determine the measurement error for your sample
 
4
 
Calculation of Measurement Uncertainty
 
Notes:
Interferometer accuracy is on the order of 
λ
/50 (
δ
m = 0.02)
Wavelength uncertainty is typically small and does not contribute much error
Best uncertainty is achieved by making the sample as thick as possible while
maintaining the ability to resolve fringes (see next slide)
 
5
 
Calculation of Fringe Density
 
m
 = # of fringes
λ
 = wavelength
t
 = thickness
 
The fringe density limits the
thickness of the sample
Thicker samples will eventually
reach a fringe density that
cannot be resolved
Use calculator below to estimate
fringe density in your samples
 
Notes:
For wavelengths in the visible
and NIR, the maximum fringe
density that can be resolved by
the interferometer is 
100 mm
-1
Samples with large fringe density
will require a smaller field of
view
Stitching may be required to
measure the full sample
 
6
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Mach-Zehnder Interferometer is a powerful tool used by the University of Rochester Gradient-Index Research Group for measuring 2-D Gradient-Index (GRIN) profiles. This instrument covers a wavelength range of 0.355 to 12 µm with high measurement accuracy. The sample preparation involves thin, parallel samples with exposed GRIN, and measurement uncertainty is determined by factors like surface figure error and wedge. The calculation of measurement uncertainty is essential for accurate GRIN profile measurements.

  • Mach-Zehnder Interferometer
  • 2-D GRIN Profile
  • University of Rochester
  • Measurement Uncertainty
  • Gradient-Index Research

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  1. Mach-Zehnder Interferometer for 2-D GRIN Profile Measurement Instrument Overview Sample Preparation Measurement Uncertainty University of Rochester Gradient-Index Research Group

  2. 2D GRIN Measurement: Mach-Zehnder Interferometer Wavelength range covered 0.355 1.064 m, 1.55 4.6 m, 8 12 m Measurement accuracy ( n) = 1E-5 Beam size: 65mm x 40mm ellipse Sample prep requirements Thin (~1mm), plane, parallel sample with GRIN exposed (index is constant through sample thickness) Laser Spatial Filter Mirror Beam Splitter Beam Splitter Sample 2 ( )t = ( , ) ( , ) x y n x y Mirror Measure: , t Calculate: n Lens Detector Measured Interferogram Measurement Slice GRIN Blank 2

  3. Mach-Zehnder Sample Prep Measurement Slice Measured Interferogram GRIN Blank t = = # of Fringes N n Radial Sample thickness chosen so that # of fringes can be resolved by imaging optics and detector Surface figure error and wedge lead to measurement error y x Axial Thin slice cross-section that exposes the gradient for measurement Index should be constant through the thickness of the sample (z-axis) 3

  4. Mach-Zehnder Measurement Uncertainty m = # of fringes = wavelength t = thickness m = n t Best-case uncertainty is determined by a root-sum-square of the terms in the n calculation 2 2 2 t m m = + + ( ) n m t t t 2 Uncertainty is increased further by surface figure error and wedge, but it can be minimized by measuring in an index matching fluid Uncertainty due to: Expression t - Figure error measured in air - Wedge error if no known homogeneous region = ) 1 ( ) ( n n samp t t = ( ) ( ) n n n - Figure error measured in fluid samp fluid t - Figure error measured in matched fluid (nfluid = nsamp at some location in sample) - Wedge error if there is a known homogeneous region t = ( ) n n t Use the calculator on the next slide to determine the measurement error for your sample 4

  5. Calculation of Measurement Uncertainty RSS uncertainty Best-case measurement uncertainty m m 0.02 t ( m) 1500 t ( m) 0.6328 0.00005 Sample Prep Errors 35 nsamp sample n nfluid t ( m) 1.78 0.03 1.7 1 1 = 1.58 waves ( = 0.632 m) Figure Error in Fluid ( n) ( n) 1.302E-05 5.33E-05 Figure Error in Matched Fluid (or wedge if known homog. Region) ( n) 2.00E-05 User Input Calculated Value Figure Error in Air (or wedge if no known homog. Region) ( n) 5.20E-04 Notes: Interferometer accuracy is on the order of /50 ( m = 0.02) Wavelength uncertainty is typically small and does not contribute much error Best uncertainty is achieved by making the sample as thick as possible while maintaining the ability to resolve fringes (see next slide) 5

  6. Calculation of Fringe Density The fringe density limits the thickness of the sample Thicker samples will eventually reach a fringe density that cannot be resolved Use calculator below to estimate fringe density in your samples m = # of fringes = wavelength t = thickness m = n t t = = # of Fringes N n thickness ( m) wavelength ( m) sample n spatial extent of gradient (mm) 1500 0.6328 0.03 Notes: For wavelengths in the visible and NIR, the maximum fringe density that can be resolved by the interferometer is 100 mm-1 Samples with large fringe density will require a smaller field of view Stitching may be required to measure the full sample 1.2 index slope (mm-1) # of fringes fringe density (mm-1) 0.02500 71.1 59.3 User Input Calculated Value 6

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