Abstract

Figures of merit for comparing various holographic storage media are defined and discussed. These figures of merit are based on the dynamic range of the medium. Formulas for these figures of merit are derived for photographic film.

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  1. G. W. Stroke, An Introduction to Coherent Optics and Holography (Academic Press Inc., New York, 1966), p. 116.
  2. L. J. Cutrona, E. Leith, C. Palermo, and L. Porcello, IRE Trans. IT-6, 139 (1964).
  3. D. Falconer, J. Soc. Phot. Sci. Eng. 10, 133 (1966).
  4. A. Kozma, J. Opt. Soc. Am. 56, 428 (1966).
  5. A. Vander Lugt and R. H. Mitchel, J. Opt. Soc. Am. 57, 372 (1967).
  6. J. W. Goodman, J. Opt. Soc. Am. 57, 483 (1967).
  7. A. Kozma, J. Opt. Soc. Am. 58, 436 (1968).
  8. O. Bryngdahl and A. Lohmann, J. Opt. Soc. Am. 58, 1325 (1968).
  9. The object length XB-XA must be no greater3 than (XB+XA)/3. This requirement is equivalent to limiting the fractional spatial-frequency bandwidth of the hologram to two thirds.
  10. Additional ghost images appear in the reconstruction but they may be shown to have negligible irradiances.
  11. A. A. Friesem, A. Kozma, and G. F. Adams, Appl. Opt. 6, 851 (1967).
  12. We assume, in this small-signal calculation, that the term (4H0/K1)[K2+3K3 (HR+3H0)]≪1 [see Eq. (5)].
  13. We note, however, that the effect of the assumption is to yield a value of Hmax that is somewhat larger than it ought to be. This, in turn, leads us to interpret Eq. (12) as an upper bound on dynamic range.

Adams, G. F.

A. A. Friesem, A. Kozma, and G. F. Adams, Appl. Opt. 6, 851 (1967).

Bryngdahl, O.

O. Bryngdahl and A. Lohmann, J. Opt. Soc. Am. 58, 1325 (1968).

Cutrona, L. J.

L. J. Cutrona, E. Leith, C. Palermo, and L. Porcello, IRE Trans. IT-6, 139 (1964).

Falconer, D.

D. Falconer, J. Soc. Phot. Sci. Eng. 10, 133 (1966).

Friesem, A. A.

A. A. Friesem, A. Kozma, and G. F. Adams, Appl. Opt. 6, 851 (1967).

Goodman, J. W.

J. W. Goodman, J. Opt. Soc. Am. 57, 483 (1967).

Kozma, A.

A. Kozma, J. Opt. Soc. Am. 58, 436 (1968).

A. A. Friesem, A. Kozma, and G. F. Adams, Appl. Opt. 6, 851 (1967).

A. Kozma, J. Opt. Soc. Am. 56, 428 (1966).

Leith, E.

L. J. Cutrona, E. Leith, C. Palermo, and L. Porcello, IRE Trans. IT-6, 139 (1964).

Lohmann, A.

O. Bryngdahl and A. Lohmann, J. Opt. Soc. Am. 58, 1325 (1968).

Lugt, A. Vander

A. Vander Lugt and R. H. Mitchel, J. Opt. Soc. Am. 57, 372 (1967).

Mitchel, R. H.

A. Vander Lugt and R. H. Mitchel, J. Opt. Soc. Am. 57, 372 (1967).

Palermo, C.

L. J. Cutrona, E. Leith, C. Palermo, and L. Porcello, IRE Trans. IT-6, 139 (1964).

Porcello, L.

L. J. Cutrona, E. Leith, C. Palermo, and L. Porcello, IRE Trans. IT-6, 139 (1964).

Stroke, G. W.

G. W. Stroke, An Introduction to Coherent Optics and Holography (Academic Press Inc., New York, 1966), p. 116.

Other (13)

G. W. Stroke, An Introduction to Coherent Optics and Holography (Academic Press Inc., New York, 1966), p. 116.

L. J. Cutrona, E. Leith, C. Palermo, and L. Porcello, IRE Trans. IT-6, 139 (1964).

D. Falconer, J. Soc. Phot. Sci. Eng. 10, 133 (1966).

A. Kozma, J. Opt. Soc. Am. 56, 428 (1966).

A. Vander Lugt and R. H. Mitchel, J. Opt. Soc. Am. 57, 372 (1967).

J. W. Goodman, J. Opt. Soc. Am. 57, 483 (1967).

A. Kozma, J. Opt. Soc. Am. 58, 436 (1968).

O. Bryngdahl and A. Lohmann, J. Opt. Soc. Am. 58, 1325 (1968).

The object length XB-XA must be no greater3 than (XB+XA)/3. This requirement is equivalent to limiting the fractional spatial-frequency bandwidth of the hologram to two thirds.

Additional ghost images appear in the reconstruction but they may be shown to have negligible irradiances.

A. A. Friesem, A. Kozma, and G. F. Adams, Appl. Opt. 6, 851 (1967).

We assume, in this small-signal calculation, that the term (4H0/K1)[K2+3K3 (HR+3H0)]≪1 [see Eq. (5)].

We note, however, that the effect of the assumption is to yield a value of Hmax that is somewhat larger than it ought to be. This, in turn, leads us to interpret Eq. (12) as an upper bound on dynamic range.

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