Deflection and stress analysis of a 42-m diam primary mirror of an altazimuth-mounted telescope
- 15 March 1980
- journal article
- Published by Optica Publishing Group in Applied Optics
- Vol. 19 (6) , 1000-1010
- https://doi.org/10.1364/ao.19.001000
Abstract
Large finite-element mathematical models are developed to calculate the deformations induced by the supports of a 4.2-m aperture 3.2-focal ratio primary mirror of an optical telescope. It is supported axially on three rings of pneumatic cylinders and radially by a system of transverse level weights, an arrangement only possible in a telescope that uses an altazimuth mounting. The stress distributions in the mirror when lifted by a central lifter and when resting on its axial flotation system are shown. A comparison is made between the results using classical flat-plate theory and the finite-element models.Keywords
This publication has 5 references indexed in Scilit:
- Theoretical Elastic Deformations of the Steward Observatory 230-cm and the Optical Sciences Center 154-cm MirrorsApplied Optics, 1972
- Theoretical Elastic Deflections of a Thick Horizontal Circular Mirror on a Ring SupportApplied Optics, 1970
- Theoretical Elastic Deformations of a 4-m Diameter Optical Mirror Using Dynamic RelaxationApplied Optics, 1968
- DYNAMIC RELAXATIONProceedings of the Institution of Civil Engineers, 1966
- Optical Effect of Flexure in Vertically Mounted Precision MirrorsJournal of the Optical Society of America, 1954