Sector servo system for high speed seeking and high track density

1988 ◽  
Vol 24 (6) ◽  
pp. 2955-2957 ◽  
Author(s):  
T. Yamada ◽  
T. Inoue ◽  
T. Sugaya
2002 ◽  
Vol 8 (2-3) ◽  
pp. 161-168 ◽  
Author(s):  
S.-M. Suh ◽  
C. C. Chung ◽  
S.-H. Lee

2009 ◽  
Vol 129 (3) ◽  
pp. 235-242 ◽  
Author(s):  
Masaki Sazawa ◽  
Kiyoshi Ohishi ◽  
Seiichiro Katsura

2002 ◽  
Vol 68 (668) ◽  
pp. 1191-1197
Author(s):  
Masatoshi HIKIZU ◽  
Hiroaki SEKI ◽  
Yoshitsugu KAMIYA ◽  
Hiroshi TACHIYA ◽  
Hisanao NOMURA

2009 ◽  
Vol 45 (10) ◽  
pp. 3558-3561 ◽  
Author(s):  
S. Das ◽  
N. Ito ◽  
M. Sugiyama ◽  
K. Nakamoto
Keyword(s):  

IEEE Access ◽  
2020 ◽  
Vol 8 ◽  
pp. 129799-129812
Author(s):  
Gang Yang ◽  
Peng Jiang ◽  
Lei Lei ◽  
Yong Wu ◽  
Jingmin Du ◽  
...  

Author(s):  
Mohamed Slamani ◽  
Albert Nubiola ◽  
Ilian A. Bonev

Two important aspects of the performance of a servo system, tracking errors and contour errors, significantly affect the accuracy of industrial robots under high-speed motion. Careful tuning of the control parameters in a servo system is essential, if the risk of severe structural vibration and a large contouring error is to be avoided. In this paper, we present an overview of a method to diagnose contouring errors caused by the servo control system of an ABB IRB 1600 industrial robot by measuring the robot’s motion accuracy in a Cartesian circular shape using a double ballbar (DBB) measurement instrument. Tests were carried out at different TCP (tool centre-point) speed and trajectory radii to investigate the main sources of errors that affect circular contouring accuracy. Results show that radius size errors and out-of-roundness are significant. A simple experimental model based on statistical tests was also developed to represent and predict the radius size error. The model was evaluated by comparing its prediction capability in several experiments. An excellent error prediction capability was observed.


1986 ◽  
Vol 118 ◽  
pp. 121-122
Author(s):  
Wan Lai ◽  
Zhu Neng-hong ◽  
Wang Lan-juan ◽  
Yang Zheng-hua ◽  
Zheng Yi-jin

This telescope was designed for determining the trigonometric parallaxes of faint stars. The otpical configuration is a Ritchey-Chrétien system and has only a f/10 Cassegrain focus for photographic work.The mounting is a combination of fork and yoke frame which can reduce the flexure due to gravity. A high speed digital servo-system was adopted for controlling and driving the telescope. At present some photographs of Comet Halley have been obtained.


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