QC 351 A7 no. 06 / A 6-inch aperture 3-mirror optical system has been designed that
yields high resolution over a flat field of 6° at a speed of f/1.8. All
surfaces are strongly aspheric. A proposed application of this new type
of camera is for sky survey and stellar photographic photometry in the
far ultraviolet under a current NASA Apollo AAP program. A general discussion of 3-mirror reflective systems is given.
Identifer | oai:union.ndltd.org:arizona.edu/oai:arizona.openrepository.com:10150/621601 |
Date | January 1966 |
Creators | Meinel, Aden B., Shack, Roland V. |
Publisher | Optical Sciences Center, University of Arizona (Tucson, Arizona) |
Source Sets | University of Arizona |
Language | en_US |
Detected Language | English |
Type | Technical Report |
Rights | Copyright © Arizona Board of Regents |
Relation | Optical Sciences Technical Report 06 |
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