Two-Wavelength Papers
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Katherine Creath and James C. Wyant
Proceedings
of SPIE,
Vol. 645, page 101, 1986
Two-wavelength holography and phase-shifting
interferometry are combined to measure aspheric surface contours with
variable sensitivity. In this technique, the surface is effectively
tested at a synthesized longer equivalent wavelength leq=la
lb/Abs[la
- lb] using measurements made at
wavelengths la and
lb where the difference of the phases measured for
la and lb
yields modulo 2p phase at leq.
A mask of point apertures is placed over the detector array in order to
resolve closely spaced fringes. This technique has an rms
repeatability of leq/100. Limits
to this technique are discussed and results are shown. |
Katherine Creath, Yeou-Yen Cheng, and James C.
Wyant
Optica Acta, Vol. 32, page 1455, 1985
Two-wavelength holography and phase-shifting interferometry are combined to
measure the phase contours of deep wavefronts and surfaces, such as those produced by
aspherics, with a variable sensitivity. When interference fringes are very closely spaced,
the phase data contain high frequencies where 2p ambiguities
cannot be resolved. In this technique, the surface is tested at a synthesized longer
equivalent wavelength. The phase of the wavefront is calculated modulo 2p
using phase-shifting techniques at each of two visible wavelengths. The difference
between these two phase sets is the phase of the wavefront as it would be measured at leq =l1l2/|l1-l2|, assuming that 2p ambiguities can be removed at leq. This
technique enables surfaces to be contoured to an accuracy of leq/l00. |
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Yeou-Yen Cheng and James C. Wyant
APPLIED OPTICS, Vol. 24, page 804, 15 March 1985
This paper describes a method to
enhance the capability of two-wavelength phase-shifting interferometry. By
introducing the phase data of a third wavelength, one can measure the phase of a very
steep wave front. Experiments have been performed using a linear detector array to
measure surface height of an off-axis parabola. For the wave front being measured
the optical path difference between adjacent detector pixels was as large as 3.3 waves.
After temporal averaging of five sets of data, the repeatability of the measurement is
better than 25-Å rms (l = 6328 Å).
URL:
http://www.opticsinfobase.org/abstract.cfm?URI=ao-24-6-804 |
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Yeou-Yen Cheng and James C. Wyant
APPLIED OPTICS, Vol. 23, page
4539, 15 December 1984
This paper
describes a technique that combines ideas of phase
shifting interferometry (PSI) and two-wavelength interferometry (TWLI) to
extend the phase measurement range of conventional single-wavelength PSI.
To verify theoretical predictions, experiments have been performed using a
solid-state linear detector array to measure 1-D surface heights.
Problems associated with TWLPSI and the experimental setup are discussed.
To test the capability of the TWLPSI, a very fine fringe pattern was used to
illuminate 1024 element detector array. Without temporal averaging,
the repeatability of measuring a surface having a sag of ~100mm
is better than 25-Å (0.0025%) rms.
URL:
http://www.opticsinfobase.org/abstract.cfm?URI=ao-23-24-4539 |
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J. C. Wyant, B. F. Oreb, and
P. Hariharan
APPLIED OPTICS, Vol. 23, page
4020, 15 November 1984
Two-wavelength holography has been shown to be quite
useful for testing aspheric surfaces since it can produce interferograms
with a wide range of sensitivities. However, TWH has the drawback that
the accuracy attainable from measurements on photographs of the fringes is
limited. It is shown how this limitation can be overcome by using
electronic techniques to evaluate the phase distribution in the interference
pattern.
URL:
http://www.opticsinfobase.org/abstract.cfm?URI=ao-23-22-4020 |
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Philip Lam, J.D. Gaskill, and James C. Wyant
APPLIED OPTICS, Vol. 23, page
3079, 15 September 1984
It has been demonstrated that a Bi12SiO20
crystal is a good holographic recording material. Using this crystal
as a real-time recording device, a two-wavelength holographic interferometer
has been constructed. The 488- and 514.5-nm lines of an Ar-ion laser
were used as the source to yield an equivalent wavelength of 9.47
mm.
url:
http://www.opticsinfobase.org/abstract.cfm?URI=ao-23-18-3079 |
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J. C. Wyant
APPLIED OPTICS, Vol. 10, page 2113, September 1971
It is shown that both single
exposure and double exposure two-wavelength holography provide a good method of using
visible light to obtain an interferogram identical to what would be obtained if a longer
nonvisible wavelength were used. Both techniques provide for the real-time adjustment of
defocus and tilt in the final interferogram. When both hologram exposures are made
simultaneously, the sensitivity to air turbulence is essentially the same as if the longer
nonvisible wavelength were used. Results are shown for testing both lenses and mirrors at
equivalent wavelengths at 6.45 µ, 9.47 µ, 14.20 µ, 20.22 µ, and 28.50 µ obtained by
using an argon laser for the visible light source.URL:
http://www.opticsinfobase.org/abstract.cfm?URI=ao-10-9-2113 |