1. Introduction
The use of large, light-weight, optical elements is essential for applications that
require large collecting areas but have cost or weight restrictions. One technology
under consideration for this purpose is membrane optical elements.
1
For elements of this type to be viable, methods for optically measuring
highly aberrated surface structures will need to be employed - not only for
characterization purposes, but possibly for real-time figure and surface control.
Such an optical profiling system may need to provide a spatial resolution of several
thousand points and will have to deal with aberrations ranging from hundreds of
optical waves to a fraction of a wave. In addition, a useful profilometer system
will need to be compact, light-weight, rugged, and capable of a measurement time, or
frame rate, that can approach “real-time”.
In this paper we describe a surface profiling approach that addresses the above
requirements. The fundamentals of the approach are common to those of electro-optic holography.
2
Holographic Interferometry , P.K. Rastogi, ed., Springer Ser. Opt. Sci.
68, (Springer, Berlin, 1994).
However, we have introduced a digitally-based, two-wavelength measurement
scheme to provide the interferometer with a variable sensitivity capability. Our
sensing approach employs a heterodyne phase measurement at each pixel in a CCD array
where the resulting two-dimensional map of phase values is related to the optical
path length profile of the surface under examination. This approach for surface
measurement was presented by Hariharan
3
P. Hariharan, “Quasi-heterodyne hologram interferometry,” Opt. Eng.
24, 632–638 (1985).
as “quasi-heterodyne hologram interferometry”. In that
work and most subsequent efforts
4
Y. Ishii, J. Chen, and K. Murata, “Digital phase-measuring interferometry with a tunable laser diode,” Opt. Lett.
12, 233–235 (1987). [CrossRef] [PubMed]
,5
I. Yamaguchi, J. Liu, and J. Kato, “Active phase-shifting interferometers for shape and deformation measurements,“ Opt. Eng.
35, 2930–2937 (1996). [CrossRef]
discrete phase-stepping techniques were implemented
to obtain the phase measurements. We use a continuous phase-shift approach that is
accomplished using acousto-optic modulators (AOMs).
6
D. G. Voelz, L. McMackin, J. K. Boger, and M. P. Fetrow, “Double-exposure heterodyne imaging for observing line-of-sight deformation,” Opt. Lett.
22, 1027–1029 (1997). [CrossRef] [PubMed]
Phase measurements are obtained by interfering an object and reference beam
of slightly different frequencies. The resulting temporal beat signal is sampled at
each point in the interference pattern so that the phase can be calculated. The AOMs
and associated drive circuitry can provide stable frequency shifts as small as a few
Hertz, which allows the use of an off-the-self CCD camera as the sensing element. In
general, we have found the AOM-based system to be very reliable and robust
(containing no moving parts), and simple to implement.
When hundreds of optical waves of aberration are present conventional interferometric
measurement at visible wavelengths produces too many fringes to count. Historically,
methods for optical testing in such cases have combined interferograms or holograms
that were created at two different wavelengths.
7–10
J. C. Wyant, “Testing aspherics using two-wavelength holography,” Appl. Opt.
10, 2113–2118 (1971). [CrossRef] [PubMed]
The range of optical path length that can be measured is increased using
two-wavelength techniques that create a synthetic wavelength much longer than the
optical regime. Measurement sensitivity is proportional to this equivalent
wavelength rather than the optical wavelength.
In our system a heterodyne array measurement is made for each of two different probe
laser wavelengths and each frame is stored in the computer in complex exponential
form. These digital phase frames are then differenced in the computer to produce
optical path length maps that are associated with different synthetic wavelengths. A
single tunable laser is employed that can be scanned quickly in wavelength, which
provides for nearly continuously variable-sensitivity phase measurements from which
large and small surface deviations on the same surface can be defined. As an
additional note, the advantage of working with the phase frames in a complex
exponential form in the computer is that differencing of frames, or other
multi-frame operations, can be performed without concern about 2π phase
jumps since all operations are carried out modulo-2π. Phase unwrapping is
performed only on the final result frame.
The digital super-heterodyne interferometry technique described here owes its utility
and affordability to recent advances in laser devices, CCD cameras and computer
technology. Tunable diode lasers can provide great flexibility for generating
different synthetic wavelengths. Data rates required for real-time applications can
be obtained with off-the-shelf high frame-rate CCD cameras. Frame grabbers and
PC-based computer systems now have enough memory and processing speed to handle the
data acquisition rates and phase computations required for a timely measurement.
2. Theory
The heterodyne sensing part of our concept has been described previously for an
imaging system that measures line-of-sight deformation.
6
D. G. Voelz, L. McMackin, J. K. Boger, and M. P. Fetrow, “Double-exposure heterodyne imaging for observing line-of-sight deformation,” Opt. Lett.
22, 1027–1029 (1997). [CrossRef] [PubMed]
In summary, a coherent probe beam is reflected from a test surface and
combined with a reference beam on a CCD camera. The probe and reference beams have
slightly different optical frequencies and the resulting temporally beating
intensity signal on the CCD camera is sampled and stored for each pixel. A phase
value is computed for each pixel using a simple Fourier coefficient-based algorithm.
Amplitude values at each pixel are combined with the phase information and a complex
exposure is formed in the computer. A complex exposure is given by
where r
m is a two dimensional pixel location,
λa is the illuminating wavelength,
Aa(r
m,λa) is the
product of the amplitudes of the image and reference wavefronts,
ϕa(r
m,λa) is
the phase of the test wavefront and ϕrefa is the constant
phase of the reference wavefront. The exposure has been purposely represented in a
complex exponential form because differencing or summing of different exposures can
now be done modulo-2π so that 2π phase jumps are not a
concern.
Now consider a second complex exposure measured using the illumination wavelength,
λb. This exposure is described by
In typical applications, the difference between λa and
λb may be just a few nanometers so Aa and
Ab are essentially equivalent but the phase values can be quite
different. By evaluating the following quantity in the computer, we can find the
difference between the two image phase functions,
In practice, a synchronization of the heterodyne data collection process can be
arranged so the two constant terms ϕ
refa and
ϕ
refb are equal and thus cancel,. Similarly, it is
straightforward to remove a constant value from the result in Eq. (
3). Deleting these terms leaves an
“equivalent” phase that is related to the optical path
difference (OPD) between the surface of the object and the flat reference wavefronts,
8
K. Creath, “Step height measurement using two-wavelength phase-shifting interferometry,” Appl. Opt.
26, 2810–2816 (1987). [CrossRef] [PubMed]
where
So the result in Eq. (
4) is equivalent to that of a single interferometric
measurement of the test surface using the wavelength, λ
eq.
3. Experimental setup and results
The heterodyne interferometer setup is shown in
Fig. 1. The illumination source is a diode laser that
nominally operates at a wavelength of 780 nm and is tunable over a 20-nm range with
steps as fine as 0.1 nm. After passing through some attenuation optics, the beam is
split into a probe leg and a reference leg. An acousto-optic modulator (AOM) in each
leg shifts the frequency of the beams by 40 MHz with an additional 8-Hz shift being
applied to the probe beam. Both beams are expanded and the probe beam continues on
to the test surface while the reference beam is sent to the camera face. Reflected
light from the test surface is returned to the camera face where it interferes with
the reference beam producing an 8-Hz modulated intensity signal. A standard video
rate (30 Hz) camera and frame grabber/Pentium PC system captures 16 consecutive
intensity frames from which the 8-Hz signal is demodulated for each pixel and a
complex exposure is produced (Eq. (
1)). Complex exposures at different wavelengths are obtained by
tuning the diode laser to different lines and collecting and processing accompanying
sets of intensity frames. Although not shown in
Fig. 1, it is possible to include optics in front of the
camera to form an image of the test surface or some other object at the camera face.
Fig. 1. Diagram of heterodyne array profilometer.
To test the system in the laboratory a tilted flat mirror was examined. A portion of
the mirror, approximately 6-mm square, was observed by the system and the mirror
wavefront was tilted with respect to the reference wavefront by about 70
μm/mm. This fixed surface was measured using 7 different synthetic
wavelengths generated from combinations of pairs of complex exposures (
Table 1). A sequence of the seven equivalent wavelength phase
maps produced in the lab is shown in
Fig. 2. As the equivalent wavelength increases the number of
2π phase jumps across the surface decreases. This is expected since the
tilt of the mirror wavefront is being recorded as phase values relative to the
effective wavelength. In
Fig. 3 the 2π phase jumps have been removed using
a simple phase-unwrapping routine and the phase profiles are presented as a series
of surface plots. The surface profiles show less and less slant as the equivalent
wavelength increases. In essence, the longer the effective wavelength the less
sensitive the measurement is to optical path length or depth. It is this feature
that allows optical paths of many hundreds of optical wavelengths to be measured
without counting hundreds of fringes. In
Fig. 4 the phase profile results have been scaled by the
effective wavelength to yield absolute optical path length in micrometers. In this
case the slant of the measured profile is constant at the different effective
wavelengths, which shows the mirror wavefront is not changing tilt between
measurements. As expected, the absolute measurement noise increases as the effective
wavelength increases.
2
Holographic Interferometry , P.K. Rastogi, ed., Springer Ser. Opt. Sci.
68, (Springer, Berlin, 1994).
An estimate of the fidelity of the heterodyne array phase measurement for our setup
was made by comparing two consecutive phase profiles collected with the same
wavelength (optical or effective). The phase values for the two frames were
differenced, pixel-by-pixel, and then the standard deviation of this error over the
640 × 480 pixels was calculated. For the single optical wavelength
measurement this standard deviation was typically about λ/120. For the
effective wavelength measurements the standard deviation ranged from about
λeq/60 for λeq=40 μm to
λeq/70 for λeq=600 μm.
Table 1. Complex exposure wavelengths and resulting equivalent wavelengths
| λa (μm) | λb (μm) | λeq (μm) |
|---|
| 0.792 | 0.7766 | 40 |
| 0.792 | 0.7817 | 60 |
| 0.792 | 0.7842 | 80 |
| 0.792 | 0.7858 | 100 |
| 0.792 | 0.7889 | 200 |
| 0.792 | 0.7910 | 600 |
| 0.792 | 0.7912 | 800 |
Fig. 2. Phase maps of a tilted surface for the equivalent wavelengths in
Table 1. [
Media 1]
Fig. 3. Unwrapped phase profile plots of a tilted surface for the equivalent
wavelengths in
Table 1. [
Media 2]
Fig. 4. Optical path profiles of a tilted surface for the equivalent wavelengths in
Table 1. [
Media 3]
4. Summary
The multiple wavelength heterodyne array profilometer described and demonstrated here
has the following strengths: 1) the use of multiple wavelengths generated by a diode
laser provides for a large and variable range of optical path length measurement, 2)
the heterodyne phase sensing approach is easily implemented with simple, compact and
reliable hardware, and 3) wavefronts can be measured with high phase resolution as
well as high, two-dimensional, spatial resolution. These attributes make this
wavefront sensing approach attractive for measuring the surface structure and
wavefront quality of large, highly aberrated optics. The heterodyne array sensing
approach holds promise for high-speed phase measurement without sacrificing spatial
or phase resolution. This promise stems from the fact that the phase processing is
inherently a parallel operation involving no cross-pixel calculations and is simple
enough in principle to be implemented in a digital or analog fashion on a sensor
chip. The possibility of rapid wavefront measurement makes this approach of interest
for “real-time” control of adaptive optical systems.
In addition to the innovation of combining heterodyne array sensing with multiple
wavelength measurements, we also employ the approach of working with the digital
complex exposures in the computer in a complex exponential form. The differencing of
complex exposure frames, or other multi-frame linear operations of interest, can be
performed as complex exponentials without concern about 2π phase jumps
since all operations are carried out modulo-2π.
Acknowledgments
The authors thank Laura Ulibarri, Mervyn Kellum, and Ken MacDonald for assisting with
the laboratory measurements and data processing.
References and Links
1. |
D. K. Marker and C. H. Jenkins, “Surface precision of optical membranes with curvature,” Opt. Express
1, 324–331 (1997). http://epubs.osa.org/oearchive/source/2668.htm [CrossRef] [PubMed] |
2. |
Holographic Interferometry , P.K. Rastogi, ed., Springer Ser. Opt. Sci.
68, (Springer, Berlin, 1994). |
3. |
P. Hariharan, “Quasi-heterodyne hologram interferometry,” Opt. Eng.
24, 632–638 (1985). |
4. |
Y. Ishii, J. Chen, and K. Murata, “Digital phase-measuring interferometry with a tunable laser diode,” Opt. Lett.
12, 233–235 (1987). [CrossRef] [PubMed] |
5. |
I. Yamaguchi, J. Liu, and J. Kato, “Active phase-shifting interferometers for shape and deformation measurements,“ Opt. Eng.
35, 2930–2937 (1996). [CrossRef] |
6. |
D. G. Voelz, L. McMackin, J. K. Boger, and M. P. Fetrow, “Double-exposure heterodyne imaging for observing line-of-sight deformation,” Opt. Lett.
22, 1027–1029 (1997). [CrossRef] [PubMed] |
7. |
J. C. Wyant, “Testing aspherics using two-wavelength holography,” Appl. Opt.
10, 2113–2118 (1971). [CrossRef] [PubMed] |
8. |
K. Creath, “Step height measurement using two-wavelength phase-shifting interferometry,” Appl. Opt.
26, 2810–2816 (1987). [CrossRef] [PubMed] |
9. |
R. Dandliker, R. Thalmann, and D. Prongue, “Two-wavelength laser interferometry using superheterodyne detection,” Opt. Lett.
13, 339–341 (1988). [CrossRef] [PubMed] |
10. |
E. Gelmini, U. Minoni, and F. Docchio, “Tunable, double wavelength heterodyne detection interferometer for absolute distance measurements,” Opt. Lett.
19, 213–215 (1994). [CrossRef] [PubMed] |