Ultra-low speed research on friction drive for astronomical telescope
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Ultra-low speed research on friction drive for astronomical telescope
Optics and Precision EngineeringVol. 14, Issue 2, Pages: 274-278(2006)
作者机构:
1. 中国科学院研究生院
2. 中国科学院 国家天文台 南京天文光学技术研究所,江苏 南京210042
作者简介:
基金信息:
DOI:
CLC:TH751
Received:22 December 2005,
Revised:16 January 2006,
Published Online:30 April 2006,
Published:30 April 2006
稿件说明:
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WANG Da-xing, DU Fu-jia. Ultra-low speed research on friction drive for astronomical telescope[J]. Optics and precision engineering, 2006, 14(2): 274-278.
DOI:
WANG Da-xing, DU Fu-jia. Ultra-low speed research on friction drive for astronomical telescope[J]. Optics and precision engineering, 2006, 14(2): 274-278.DOI:
Ultra-low speed research on friction drive for astronomical telescope
The theory and characteristics of friction drive for a large astronomical telescope were presented. The results of experiment indicate that there are many factors influencing on the stability of low speed of friction drive. The main factors include:measuring error of encoder ;error of environment variance;errors of friction torque and motor fluctuating torque and error of manufacturing and installing. In addition
the friction torque of total drive chain is fluctuation also. The results of experiments also indicate that the nonlinear characteristic of increment parameter of nonlinear PID control algorithm can achieve prompt response and non-overshooting of the control system. The nonlinear PID also enhances the stability to resist the influence of friction drive low speed. In this experiment
the low speed is 0.2″/s and position precision is 0.032″(RMS)
which proved that this method is effective.
关键词
Keywords
references
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