The Digital Motion Control System for the Submillimeter Array Antennas

• Published in: arXiv.org
• Main Authors: Hunter, T R, Wilson, R W, Kimberk, R, Leiker, P S, Patel, N A, Blundell, R, Christensen, R D, Diven, A R, Maute, J, Plante, R J, Riddle, P, Young, K H
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 18.03.2013
• Subjects: Acceleration; Algorithms; Amplifiers; Antenna arrays; Brushless motors; Coders; Computer memory; Control systems; Control theory; Elevation; Error functions; Microcontrollers; Motion control; Parabolic antennas; Physics - Instrumentation and Methods for Astrophysics; Product design; Proportional integral derivative; Receivers & amplifiers; Remote monitoring; Servocontrol; Shutdowns; Software; Tachometers; Torque; Touch screens; UNIX
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.1303.4397

We describe the design and performance of the digital servo and motion control system for the 6-meter diameter parabolic antennas of the Submillimeter Array (SMA) on Mauna Kea, Hawaii. The system is divided into three nested layers operating at a different, appropriate bandwidth. (1) A rack-mounted, real-time Unix system runs the position loop which reads the high resolution azimuth and elevation encoders and sends velocity and acceleration commands at 100 Hz to a custom-designed servo control board (SCB). (2) The microcontroller-based SCB reads the motor axis tachometers and implements the velocity loop by sending torque commands to the motor amplifiers at 558 Hz. (3) The motor amplifiers implement the torque loop by monitoring and sending current to the three-phase brushless drive motors at 20 kHz. The velocity loop uses a traditional proportional-integral-derivative (PID) control algorithm, while the position loop uses only a proportional term and implements a command shaper based on the Gauss error function. Calibration factors and software filters are applied to the tachometer feedback prior to the application of the servo gains in the torque computations. All of these parameters are remotely adjustable in software. The three layers of the control system monitor each other and are capable of shutting down the system safely if a failure or anomaly occurs. The Unix system continuously relays antenna status to the central observatory computer via reflective memory. In each antenna, a Palm Vx hand controller displays system status and allows full local control of the drives in an intuitive touchscreen user interface. It can also be connected outside the cabin for convenience during antenna reconfigurations. Excellent tracking performance (0.3 arcsec rms) is achieved with this system. It has been in reliable operation on 8 antennas for over 10 years and has required minimal maintenance.