Calculation and Simulation Azimuth Hydrostatic Thrust Bearing of a Large Alt-Azimuth Telescope

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Abstract:

The use of hydrostatic bearing for support of telescope offers a number of potential performance advantages, but the structure parameter of bearing is the main factor which influence the bearing. The temperature rise of bearing is also important for the stiffnees of the telescope mount.In addition to the known benefit of mount stiffness and tracking accuracy from exceedingly low friction, the hydrostatic bearing provides a wide range of geometric possibilities for large telescopes [1].This paper analyzes various familiar hydrostatic bearing for the azimuth and elevation axes of telescope.Theoretical calculation and simulation show that the performance of bearing meets telescope’s design requirements.The principle and process of this work and Finite Element Analysis (FEA) are introduced in detail. According to the CFX result, the structure parameter and performance of bearing ,temperature field and pressure distribution have obtained.

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28-32

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August 2013

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© 2013 Trans Tech Publications Ltd. All Rights Reserved

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[1] Donald R. Chivens, DavidE. Chivens: Impact of hydrostatic bearings on the design and performance of telescopes. Part of the SPIE Conference on Acquisition , Tracking and Pointing XIII. Oriando, Florids. April (1999).

DOI: 10.1117/12.352854

Google Scholar

[2] James Howard, David Ashby, Jonathan Kern: Performance of the Large Binocular Telescope's Hydrostatic Bearing System. SPIE Vol. 7733 773358 1-9 , (2010).

Google Scholar

[3] Douglas R Neill, Victor L Krabbendam , Mario Romero: Hydrostatic bearing arrangement for high stiffness support of the Large Synoptic Survey Telescope. SPIE, Vol. 7018 70184E 1-12, (2008).

DOI: 10.1117/12.790075

Google Scholar

[4] Steve Gunnels: The Giant Magellan Telescope (GMT) - Hydrostatic Constraints. SPIE Vol. 7733 77334Z 1-12 , (2010).

DOI: 10.1117/12.857513

Google Scholar

[5] Pierre Y. Bely: The Design and Construction of Large Optical Telescopes . Springer- verlag, (2003).

Google Scholar

[6] Wang Huai, Zhang Jingxu, Dai Shuang: Study on the Azimuth Bearing Scheme of a Large Alt-azimuth Telescope. SPIE Vol. 7654 76540Q 1-6 , (2010).

DOI: 10.1117/12.866726

Google Scholar

[7] Shengchen Yan, et al. Principle and design of hydrostatic bearing. National Defense Industry Press; 1980. p.39–42.

Google Scholar

[8] Dongju Chen, Jinwei Fan, Feihu Zhang:Dynamic and static characteristics of a hydrostatic spindle for machine tools,Journal of Manufacturing Systems 31 (2012) 26–33.

DOI: 10.1016/j.jmsy.2010.11.006

Google Scholar

[9] Jonathan de Ville, MaximePiérard, Christian Bastin: The 3. 6Indo-Belgian Devasthal Optical Telescope: The hydrostatic azimuth bearing, SPIE Vol. 8444 84443Z 1-11, (2012).

DOI: 10.1117/12.925943

Google Scholar

[10] Moaveni, S, Finite element analysis: theory and application with ANSYS. Prentice Hall PTR: (1999).

Google Scholar