Paper
15 October 1993 Cast Tenzaloy aluminum optics
Fred F. Forbes
Author Affiliations +
Proceedings Volume 1931, Metal Mirrors; (1993) https://doi.org/10.1117/12.158729
Event: Metal Mirrors, 1992, London, United Kingdom
Abstract
Since the early sixties, cast aluminum optics has held out a promise of low cost, durability, lightweight, ease of manufacture, the possibility of welding together sections to form large optics and a good match of some astronomical programs such as photometry. Needless to say, this rosy future has been fraught with difficulties. Poor short-term stability, sensitivity to temperature, porosity, bimetallic warping, soft optical surface, poor specularity, nickel adhesion problems, poor image quality, and the inability to generate aspherics, have all contributed to the bad name cast aluminum optics has acquired over the years. With the advent of improved aluminum alloys, long-term dimensional stability data, advances in adaptive optics and the need for very large monolithic mirrors with a relatively low handling risk, aluminum optics deserve another look. This paper is a collection of some of the early attempts to build cast aluminum mirrors using the stable alloy, Tenzaloy. The results of those efforts are discussed together with recommendations for future aluminum metal mirror work.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Fred F. Forbes "Cast Tenzaloy aluminum optics", Proc. SPIE 1931, Metal Mirrors, (15 October 1993); https://doi.org/10.1117/12.158729
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Cited by 2 scholarly publications.
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