2006
DOI: 10.1117/12.672139
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Use of computer generated holograms for alignment of complex null correctors

Abstract: Large diameter, non-axisymmetric aspheric mirrors can be measured interferometrically using null correctors that employ computer generated holograms (CGHs). The testing of off axis segments for the new class of giant telescopes pose requirements that beyond the state of the art for CGHs alone. The long radius of curvature and the magnitude of the aspheric departure require other lenses and mirrors to be used along with the CGH. The alignment of these systems is very sensitive and the absolute accuracy of the a… Show more

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Cited by 16 publications
(7 citation statements)
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“…8 (See Figure 5.) The 10-µm positional tolerance for the CGH and the mirror were achieved using these references.…”
Section: Heritage For Measuring Large Aspheric Mirrorsmentioning
confidence: 95%
“…8 (See Figure 5.) The 10-µm positional tolerance for the CGH and the mirror were achieved using these references.…”
Section: Heritage For Measuring Large Aspheric Mirrorsmentioning
confidence: 95%
“…Through the interferogram, we can find out whether there is tilt, defocus and decenter. If the CGH is in its nominal position, we will get a null fringe [7] . Figure 5 shows the design layout of alignment CGH.…”
Section: Alignment Cghmentioning
confidence: 99%
“…8,9 The approach is not applicable to freeform surfaces and off-axis sections of aspheres due to the missing symmetry in the illuminated surface. Burge et al 10 and Zehnder et al 11 propose projected reference marks for the alignment of the surface under test. Additional diffraction structures are placed at different positions within the illuminated aperture on the substrate or are multiplexed with the diffractive null.…”
Section: Alignment Of the Surface Under Testmentioning
confidence: 99%