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典型文献
Modeling and Measuring Friction of the Leighton 10 m Telescope
文献摘要:
Estimating and identifying friction are important aspects of simulating a mechanical drive system.Accurate friction modeling helps to improve a telescope's performance.However,the friction conditions inside are complex and hard to measure.We did simulations with mathematical transfer functions for the Leighton 10 m Telescope and employed a polyline model to identify sources of friction.We made a two-stage model for the Leighton 10 m Telescope.Based on measurements of the motor's currents and speeds,we constructed a curve containing the friction information of the transmission elements.We simulated the system using a step function input under many combinations of friction parameters.By comparing simulation results with the measured ones,we determined the various friction components.This model accurately reproduced the telescope performance including the nonlinearities.
文献关键词:
作者姓名:
Yongwei Guo;David Woody;Nicolas Matinez
作者机构:
Chinese Academy of Sciences South America Center for Astronomy,Camino El Observatorio 1515,Las Condes,Santiago,Chile;National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;California Institute of Technology,Owens Valley Radio Observatory,Big Pine,CA 93513,USA;Universidad de Concepcion,Facultad de Ciencias Físicas y Matematicas,Concepcion,403000,Chile
引用格式:
[1]Yongwei Guo;David Woody;Nicolas Matinez-.Modeling and Measuring Friction of the Leighton 10 m Telescope)[J].天文和天体物理学研究,2022(12):311-321
A类:
Leighton,polyline
B类:
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AB值:
0.600247
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