Title: Comparison of Fiber Reference and Zernike Filter Self Referencing Interferometers
1Comparison of Fiber Reference and Zernike Filter
Self Referencing Interferometers
- Kavita Chand, M.S., M.Tech, and
- Justin Mansell, Ph.D.
- MZA Associates Corporation
- Troy Rhoadarmer
- Air Force Research Laboratory
- Kirtland AFB, Albuquerque, NM
2Introduction
- Self-referencing interferometers (SRIs) have been
proposed to provide feedback for adaptive optics
systems in directed energy applications. - We performed wave-optics analysis in WaveTrain to
compare two types of SRI - Fiber-reference SRIs and
- Zernike filter SRIs.
-
3Fiber SRI
0
Aberration
Lens
p/2
Light
p
Splitter
3p/2
4WaveTrain FiberSRI
5Zernike SRI
-p/2
Aberration
Light
Lens and Splitter
p/2
- Denominator factor of 6.0 is best for weaker
aberration. - Denominator factor of 2.0 is best for stronger
aberrations.
6WaveTrain Zernike SRI
7System-Level Parametric Studies
- Types of Aberrations
- Single Phase Screen Zernike Polynomials
- Multi-Screen Distributed Atmosphere
- Types of Tests
- Intensity Debalancing
- Image Misregistration
- Tilt Rejection
- Camera Signal to Noise Ratio (SNR)
- Metric
- Used measured wrapped wavefront to compensate the
beam. - Measured Peak Strehl Ratio (PSR)
- Ratio of peak intensity in the far-field for
aberrated to that for a perfect beam
8System-Level Parametric Studies
9System-Level Parametric Studies
10System Studies with Zernike Polynomial Phase
Aberration Input
11Zernike SRI Intensity Debalancing
Used Zernike aberrations with an amplitude factor
of 2?
-p/2
x
(1-x)y
Aberration
Light
(1-x)(1-y)
Lens and Splitter
p/2
Adjusted the splitting ratio of the light into
the three arms using the variables x and y.
DF2.0
12Fiber SRI Intensity Debalancing
0
Lens
p/2
Light
p
Splitter
Aberration
3p/2
31 splitting ratio
x
Used Zernike aberrations with an amplitude factor
of 0.7?
(1-x)y
(1-x)(1-y)(1-z)
(1-x)(1-y)z
Adjusted the splitting ratio of the input light
into the four arms using the variables x, y, and
z.
13PSR for 90 Astigmatism for Zernike SRI
14PSR for 90 Astigmatism for Fiber SRI
15PSR for Various Zernikes for Zernike SRI
Results for 2nd and 3rd order Zernikes
(astigmatism, focus, coma, and trefoil)
16PSR for Various Zernikes for Fiber SRI
90 astigmatism
45 astigmatism
y trefoil
focus
x trefoil
y coma
x coma
PSR axis is from 0.5 to 1.0
17Intensity Debalancing Conclusions
- Zernike SRI is very sensitive to intensity
debalancing - PSR varied by about 40 for a 4 change in the
balancing of the 50/50 beam splitter. - Fiber SRI is fairly insensitive to intensity
debalancing - PSR varied by about 1 for a 10 change in the
balancing of the 50/50 beam splitter.
18Zernike SRI Image Misregistration
Used Zernike aberrations with an amplitude factor
of 2?
-p/2
Aberration
Light
Lens and Splitter
p/2
Adjusted the position of the images relative to
the normally centered position to simulate
cameras motion
DF2.0
19Fiber SRI Image Misregistration
0
Lens
p/2
Light
p
Splitter
Aberration
3p/2
Used Zernike aberrations with an amplitude factor
of 0.7?
Adjusted the position of the images relative to
the normally centered position to simulate
cameras motion
20PSR for 90 Astigmatism for Zernike SRI
21PSR for 90 Astigmatism for Fiber SRI
22PSR for Various Zernikes for Zernike SRI
Results for 2nd and 3rd order Zernikes
(astigmatism, focus, coma, and trefoil)
23PSR for Various Zernikes for Fiber SRI
90 astigmatism
focus
45 astigmatism
x coma
y trefoil
y coma
PSR axis is from 0.6 to 1.0
x trefoil
24Image Misregistration Conclusions
- Zernike SRI is sensitive to image misregistration
of a single image. - Although some Zernike aberrations seemed to be
more robust, most of the Zernikes saw a 20
reduction in Strehl ratio for a motion of 2 of
the beam diameter - The Fiber SRI is fairly insensitive to image
misregistration of a single image for all the
Zernikes. - Most of the Zernikes saw a 2 reduction in Strehl
ratio for a motion of 2 of the beam diameter. - 2 of the beam diameter corresponds to 160 µm on
an 8-mm diameter beam
25Setup with Camera Noise
- Number of Realizations 30
- Input Aberration is 90 degree astigmatism
- Maximum Count Value 10e9
- Eliminates effect of discretization
26Zernike SRI - Camera SNR Analysis
27Fiber SRI - Camera SNR Analysis
28SNR Conclusions
- Zernike SRI seems to be very sensitive to camera
noise. - The result might be due to the lack of frames
over which to average - Maybe a 4-bin Zernike SRI would have better noise
performance - The fiber SRI seems to be very tolerant of noise.
- The PSR dropped to 80 when the SNR was around 1.0
29System Studies with Distributed Atmosphere
30Zernike SRI Image Misregistration for Atmospheric
Aberrations Setup
- We are using tilt-removed model of the
atmosphere. - D / r0 1,2,3,4,5
- Range 2.0 m
- Fresnel Number 5
- Denominator Factor
- 6 for D / r0 1, 2, and 3 .
- 2 for D / r0 4, and 5 .
- Number of screens 3
- Number of Realizations 9
31Zernike SRI Image Misregistration
1
0.9
Average Peak Strehl Ratio
0.8
D / r0 5 DF 2
0.7
0.6
0.5
0.4
0.3
0.2
0.01
0.05
0.06
0.07
-0.01
0
0.04
0.03
0.02
dy/Dbeam
Error bars are standard deviation
32Fiber SRI Image Misregistration
1
0.9
0.8
Average Peak Strehl Ratio
0.7
0.6
0.5
0.4
0.3
0.2
DoverR0 5
0.1
0
0.02
0.04
0.06
0.08
0.1
-0.02
0
0.12
dy/Dbeam
Error bars are standard deviation
33Zernike SRI Image Misregistration
PSR is averaged over 9 realizations
D/r0 4
34Fiber SRI Image Misregistration
35Image Misregistration Conclusions
- For Zernike SRI, image misregistration effect
increases with increasing turbulence. - Again, the fiber SRI seems to be very insensitive
to the misalignment of a single detector.
36Zernike SRI Setup with Camera Noise
- Number of Realizations 30
- D/r0 5
- Range 2 m
- Fresnel number 5
- Maximum Count Value 10e9
- Eliminates the effect of discretization
37Zernike SRI - Camera Noise
D / r0 5
38Fiber SRI - Camera Noise
D / r0 5
39Atm. Camera Noise Conclusions
- The Zernike SRI is sensitive to noise, but not as
bad as with the astigmatism term tested earlier. - Again the noise performance seems to be better
for the fiber SRI than for the Zernike SRI.
40System-Level Parametric Studies
41SRI Comparison Overview
- In almost every comparison between the 3-bin
Zernike SRI and the 4-bin fiber SRI, the fiber
SRI had better performance. - Future Work
- Compare a 4-bin fiber SRI to a 4-bin Zernike SRI.
- Complete rigorous AO study with both devices.
42Questions?
43Backup Slides
44Peak Strehl Ratio
45Intensity Debalancing
DoverR0 3
46Mesh Parameters for FiberSRI
Effective Focal Length 37.4 mm Fiber Waist
5.2 µm Wavelength 1.55 µm Aperture diameter 8
mm
NOTE Determined using Steve Coys theory of mesh
parameters.
47Mesh Parameters for Zernike SRI
Effective Focal Length 1 m Turbulence Strength
2.6 Wavelength 1.55e-06 m Aperture diameter
8mm
NOTE Determined using Steve Coys theory of mesh
parameters.
48New Test System Components
- Ideal Compensator
- Used to apply the conjugate of the measured phase
to the beam. - Operates like an ideal deformable mirror.
- Peak Strehl Ratio Meter
- Used to calculate the ratio of the peak intensity
of the far-field spot with the residual
aberration remaining after ideal compensation to
that without any aberration. - We also used on-axis Strehl ratio which was
calculated using the discrete version of the
integral form.
49Fiber SRI Intensity Debalancing for Atmospheric
Aberrations Setup
- We are using tilt-removed model of atmosphere
- Range 3.45 m
- Frenel number 3
- Number of Screens 3
- Number of Realizations 8
- Data is recorded for low ,medium and high
turbulence. - - D/r0 1,2,3,4,5
50Fiber SRI Intensity Debalancing Conclusions
- Often saw increase in performance by adjusting
splitting ratios. - Saw a similar result with Zernike SRI
- More investigation needs to be done here to
determine the reason for this effect.
51Image Misregistration Setup
- We are using tilt-removed model of the
atmosphere. - D / r0 1,2,3,4,5
- Denominator Factor
- 6 for D / r0 1, 2, and 3 .
- 2 for D / r0 4, and 5 .
- Moving Image at 4 bin processing from 0 to 0.6
times input beam diameter. - Number of Screens 3