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Journal of the Optical Society of America

Journal of the Optical Society of America

  • Vol. 58, Iss. 3 — Mar. 1, 1968
  • pp: 436–438

Effects of Film-Grain Noise in Holography*

ADAM KOZMA  »View Author Affiliations


JOSA, Vol. 58, Issue 3, pp. 436-438 (1968)
http://dx.doi.org/10.1364/JOSA.58.000436


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Citation
ADAM KOZMA, "Effects of Film-Grain Noise in Holography*," J. Opt. Soc. Am. 58, 436-438 (1968)
http://www.opticsinfobase.org/josa/abstract.cfm?URI=josa-58-3-436


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References

  1. J. W. Goodman, J. Opt. Soc. Am. 57, 493, (1967).
  2. E. T. Whittaker and G. N. Watson, Modern Analysis, 4th Edition (Cambridge University Press, London. 1927), p. 65.
  3. A. A. Friesem, A. Kozma, and G. Adams, Appl. Opt. 6, 861 (1967).
  4. The curve is normalized in such a way that a unit exposure, which in this case is taken to be the exposure produced by the reference beam, produces a transmittance which is centered on the linear portion of the Ta-E curve.
  5. W. B. Davenport, Jr. and W. L. Root, Random Signals and Noise (McGraw-Hill Book Company, New York, 1958), p. 183.
  6. This is analogous to electrical time signals, where the frequency bandwidth of the measurement filter must be much greater than the reciprocal of the measurement time to provide a good estimate of the power spectrum. See, for instance, R. B. Blackman and J. W. Tukey, .Measurement of Power Spectra (Dover Publications, Inc., New York, 1958).
  7. E. N. Leith, Phot. Sci. Eng. 6, 75 (1962).
  8. C. B. Burckhardt, J. Opt. Soc. Am. 56, 1449A (1966).
  9. Burckhardt gives values for Φr′r′(ƒ) from 200 l/mm to 750 l/mm. We assume that the experimental curve may be extrapolated to lower and higher spatial frequencies.

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