Abstract

A straightforward graphical procedure for the design of light baffles for cassegrainian optical systems has been developed. It is completely general and generates all of the paraxial parameters from a minimum of input data.

© 1968 Optical Society of America

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References

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  1. A. Bouwers, Achievements in Optics (Elsevier Publishing Company, Inc., New York, 1950).
  2. F. Sauer, Sterne u. Weltraum 4, 141 (1966).
  3. A. T. Young, Appl. Opt. 6, 1063 (1967).
    [CrossRef] [PubMed]
  4. J. R. Golin, Avco Research Laboratory, in preparation.
  5. R. R. Willey, Sky and Telescope 25, 232 (1963).

1967 (1)

1966 (1)

F. Sauer, Sterne u. Weltraum 4, 141 (1966).

1963 (1)

R. R. Willey, Sky and Telescope 25, 232 (1963).

Bouwers, A.

A. Bouwers, Achievements in Optics (Elsevier Publishing Company, Inc., New York, 1950).

Golin, J. R.

J. R. Golin, Avco Research Laboratory, in preparation.

Sauer, F.

F. Sauer, Sterne u. Weltraum 4, 141 (1966).

Willey, R. R.

R. R. Willey, Sky and Telescope 25, 232 (1963).

Young, A. T.

Appl. Opt. (1)

Sky and Telescope (1)

R. R. Willey, Sky and Telescope 25, 232 (1963).

Sterne u. Weltraum (1)

F. Sauer, Sterne u. Weltraum 4, 141 (1966).

Other (2)

A. Bouwers, Achievements in Optics (Elsevier Publishing Company, Inc., New York, 1950).

J. R. Golin, Avco Research Laboratory, in preparation.

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Figures (1)

Fig. 1
Fig. 1

This figure identifies the various first-order parameters defined in the text. All primed umbers refer to lines which are parallel to the line with the same number unprimed. The line through a, a represents the limiting ray due to the baffles drawn in heavily along rays 5 and 6. The shading represents the limits of the baffle cross section.

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