Three-Mirror Anastigmat Telescope with an Unvignetted Flat Focal Plane
Author(s) -
Kyoji Nariai,
Masanori Iye
Publication year - 2005
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/57.2.391
Subject(s) - vignetting , physics , optics , magnification , reflecting telescope , cardinal point , telescope , curved mirror , field of view , plane mirror , aperture (computer memory) , cassegrain reflector , secondary mirror , entrance pupil , focal length , schmidt camera , lens (geology) , primary mirror , pupil , acoustics
A new optical design concept of telescopes to provide an aberration-free,wide field, unvignetted flat focal plane is described. The system employs threeaspheric mirrors to remove aberrations, and provides a semi-circular field ofview with minimum vignetting. The third mirror reimages the intermediate imagemade by the first two-mirror system with a magnification factor on the order ofunity. The present system contrasts with the Korsch system where themagnification factor of the third mirror is usually much larger than unity. Twoseparate optical trains can be deployed to cover the entire circular field, ifnecessary.Comment: 13 pages, 6 figures, 2 table
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