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The Ultra-low Speed Research on Friction Drive of Large telescope
Fujia DU; Daxing WANG
2006-06-27
Source PublicationAdvanced Software and Control for Astronomy
Volume6274
Issue6274
PagesVol.6274 10-1-10
Conference Date2006-5-24
Conference PlaceOrlando, FL
Funding OrganizationThe International Society for Optical Engineering
PublisherSPIE
Abstract
No periodical error and free of backlash are the main advantages of friction drive. So friction drive is applied in many ultra-low speed systems in the past years. With the trend that the aperture of optical telescope becomes bigger and bigger, there are some reports about friction drive employed to drive the telescopes. However friction drive also brings up challenge to control system because the inherent nonlinear characteristics of friction drive. This report describes the study on the friction drive finished in an experiment arranged by LAMOST project. It comprises three main parts. First, it introduces the experiment apparatus and presents a friction nonlinear curve to indicate the nonlinear characteristics of friction drive. Subsequently, this report illuminates the negative result that influenced by the nonlinear characteristic. Secondly, this report use nonlinear PID control algorithm to control friction drive. It achieves ultra-low speed and high precision position control. The ultra-low velocity is 0.2″/S and error is 0.032″(RMS). This report also lists some factors that influence the precision of speed. Lastly, this report gives the analysis fluctuating speed of friction drive and applies acceleration feedback to diminish this fluctuating.
KeywordLarge Telescope Friction Drive, Ultra-low Speed Nonlinear Pid Control
Subject Area精密机械及传动 ; 自动控制
Document Type会议论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/457
Collection中国科学院南京天文光学技术研究所_会议论文
望远镜新技术研究室_会议论文
Recommended Citation
GB/T 7714
Fujia DU,Daxing WANG. The Ultra-low Speed Research on Friction Drive of Large telescope[C]:SPIE,2006:Vol.6274 10-1-10.
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