Hostname: page-component-7479d7b7d-68ccn Total loading time: 0 Render date: 2024-07-09T07:26:54.932Z Has data issue: false hasContentIssue false

A Systematic Review of Aperture Shapes

Published online by Cambridge University Press:  12 April 2016

A. B. Schultz
Affiliation:
Department of Physics, University of Nevada, Reno, 89557
T. V. Frazier
Affiliation:
Department of Physics, University of Nevada, Reno, 89557

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This paper discusses the application of apodization to reflecting telescopes. The diffraction pattern of a telescope, which is the image of a star, can be changed considerably by using different aperture shapes in combination with appropriately shaped occulting masks on the optical axis. Aperture shapes studied were the circular, square, and hexagonal. Polaris (α-UMin) was used as the test system.

Type
Research Article
Copyright
Copyright © Lowell Observatory 1983

References

1. Everhart, E. and Kantorski, J. W., 1959, Astron. J., 64, 455.CrossRefGoogle Scholar
2. Jackson, J. D., 1975, Classical Electrodynamics, John Wiley & Sons, New York, 427.Google Scholar
3. Born, M. and Wolf, E., 1975, Principles of Optics, Pergamon Press, New York, 387.Google Scholar
4. Jacquinot, P. and Roizen-Dossier, B., 1964, Progress in Optics, Vol. 3 (ed. Wolf, E.; North-Holland Publishing Co., Amsterdam), 29.Google Scholar
5. van Albada, G. B., 1958, Contrib. Bosscha Obs., 1958a, No. 6, 3.Google Scholar