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Journal of the Optical Society of America

Journal of the Optical Society of America

  • Vol. 67, Iss. 3 — Mar. 1, 1977
  • pp: 393–395

Wave-front compensation error due to finite corrector-element size

Richard Hudgin  »View Author Affiliations


JOSA, Vol. 67, Issue 3, pp. 393-395 (1977)
http://dx.doi.org/10.1364/JOSA.67.000393


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Abstract

A critical component of an active optical-compensation system is the formable mirror or other phase corrector. Because the corrector will have a finite number of controllable elements, it cannot perfectly correct a distorted wave front and the resulting error must be evaluated to model and design the system properly. This paper presents the full theory of the phase corrector in two common situations: one, where a particular known type of distortion such as focus or coma is to be corrected, and two, where the distortion is a random function of position, such as might arise from atmospheric turbulence. Results for a typical corrector are presented for both situations.

© 1977 Optical Society of America

Citation
Richard Hudgin, "Wave-front compensation error due to finite corrector-element size," J. Opt. Soc. Am. 67, 393-395 (1977)
http://www.opticsinfobase.org/josa/abstract.cfm?URI=josa-67-3-393


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References

  1. R. A. Muller and A. Buffington, "Real-time correction of atmospherically degraded telescope images through image sharpening," J. Opt. Soc. Am. 64, 1200–1210 (1974).
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  3. J. W. Hard, J. Feinleib, and J. C. Wyant, in "Real-Time Phase Correction of Optical Imaging Systems," Digest of Technical Papers, Topical Meeting on Optical Propagation through Turbulence, sponsored by the OSA, ThB1-1 through ThB1-4.
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  9. J. Feinleib, S. Lipson, and P. Cone, "Monolithic Piezoelectric Mirror for Wavefront Correction," Appl. Phys. Lett. 25, 311–313 (1974).

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