WANG Guo-min, YAO Zheng-qiu, MA Li-sheng, LI Guo-ping. High precision friction drive of large telescope[J]. Editorial Office of Optics and Precision Engineering, 2004,(6): 592-597
WANG Guo-min, YAO Zheng-qiu, MA Li-sheng, LI Guo-ping. High precision friction drive of large telescope[J]. Editorial Office of Optics and Precision Engineering, 2004,(6): 592-597DOI:
A kind of optical detecting mechanism is proposed to detect the skew angle between the axes of contact roller and wheel in high precision friction drive system adopted in large astronomical telescopes. The mechanism to adjust the skew angle is also given. With the help of these mechanisms
the skew angle between roller and wheel axes is controlled below 30″. The results of experiments show that there is no skip during the movement and the friction drive can achieve high precision at ultra slow speed. The lowest long-steady velocity of the experiment drive system is 0.2″/s with corresponding precision 0.01″(RMS)
and during 30′ the lowest steady velocity is 0.05″/s with corresponding precision 0.009″(RMS). The precision of the variable velocity motion is(0.1)″(RMS)with the corresponding amplitude 30′
maximum velocity 36″/s
maximum acceleration 0.18″/s
2
. All these experiment results meet the LAMOST's specifications. The problem of object image tracked by telescope stirring in the field of view
what is more
drifting off the field of view caused by skew angle between axes of contact roller and wheel is solved by these mechanisms. The axes of roller and wheel can be kept in the ideal position in friction drive system.
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references
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