Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Investigation of the initial systems of orthoscopic astronomical objectives in the 0.2–1-µm region

Not Accessible

Your library or personal account may give you access

Abstract

This paper discusses mirror systems with an intermediate image after reflection from two mirrors, calculated for the region of third-order aberrations. The goal of this study is to search for versions with corrected distortion and acceptable values of the relative aperture of the primary mirror and the screening of the entrance pupil. The study is carried out for systems with a relative aperture of 1:6 and an angular field of 2ω=2°. A comparative analysis of mirror and mirror–lens objectives with identical optical characteristics is carried out.

© 2012 OSA

PDF Article
More Like This
An f:1.0 Camera for Astronomical Spectroscopy

Abe Offner and William B. Decker
J. Opt. Soc. Am. 41(3) 169-172 (1951)

Recent Advances in Astronomical Optics

S. C. B. Gascoigne
Appl. Opt. 12(7) 1419-1429 (1973)

Cited By

You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All Rights Reserved