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Pupil matching of Zernike aberrations |
Optics Express, Vol. 18, Issue 21, pp. 21567-21572 (2010)
http://dx.doi.org/10.1364/OE.18.021567
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Abstract
The measurement of the wavefront at the exit pupil of an optical system is a reliable method to investigate its imaging performance. It is sometimes necessary to compare the measurement obtained with a wavefront sensor to some known aberration function, which is for example given by a simulation or a gold standard measurement technique such as interferometry. For accurate measurement systems, the residual after direct subtraction of the two wavefronts is often partly due to a mismatch between coordinate systems. We present in this paper a method that uses the Zernike expansion of wavefronts to numerically cancel such small alignment errors. We use this algorithm to quantify the accuracy of a custom-built Shack-Hartmann wavefront sensor in the measurement of known aberration functions.
© 2010 Optical Society of America
OCIS Codes
(010.7350) Atmospheric and oceanic optics : Wave-front sensing
(120.3940) Instrumentation, measurement, and metrology : Metrology
(120.4800) Instrumentation, measurement, and metrology : Optical standards and testing
(220.0220) Optical design and fabrication : Optical design and fabrication
ToC Category:
Instrumentation, Measurement, and Metrology
History
Original Manuscript: July 12, 2010
Revised Manuscript: September 22, 2010
Manuscript Accepted: September 24, 2010
Published: September 27, 2010
Citation
C. E. Leroux, A. Tzschachmann, and J. C. Dainty, "Pupil matching of Zernike aberrations," Opt. Express 18, 21567-21572 (2010)
http://www.opticsinfobase.org/oe/abstract.cfm?URI=oe-18-21-21567
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References
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