Abstract

This paper discusses the design of hoods for preventing zeroth-order illumination from being incident in the focal plane of a mirror-Wright system. The hoods have the form of a tube with a port for the object beam, a central-aperture cone in a planoidal mirror, and a front screen. The shape of the port, the central-aperture cone, and the focal-plane circle is specified by two ruled surfaces, by means of which it is possible to approximately determine the geometry of the front screen.

© 2011 OSA

Optimal micro-mirror tilt angle and sync mark design for digital micro-mirror device based collinear holographic data storage system

Jinpeng Liu, Hideyoshi Horimai, Xiao Lin, Jinyan Liu, Yong Huang, and Xiaodi Tan
Appl. Opt. 56(16) 4779-4784 (2017)

A three-dimensional multispectral fluorescence optical tomography imaging system for small animals based on a conical mirror design

Changqing Li, Gregory S. Mitchell, Joyita Dutta, Sangtae Ahn, Richard M. Leahy, and Simon R. Cherry
Opt. Express 17(9) 7571-7585 (2009)

Null Test for Wright Telescope Mirrors

Edgar Everhart
Appl. Opt. 5(5) 717-718 (1966)

Wide angle mirror system design for distortionless imaging of the sky

Michael J. Kosch, Todd Pedersen, and Robert Esposito
Appl. Opt. 48(24) 4703-4708 (2009)

On the Design of Wide Angle Schmidt Optical Systems*†

Eric M. Wormser
J. Opt. Soc. Am. 40(7) 412-415 (1950)