Ziegler-Nichols frequency response method for high-order adaptive optics system of the Advanced Technology Solar Telescope

被引:0
作者
Curamen, Joseph [1 ]
Johnson, Luke [2 ]
Rimmele, Thomas [2 ]
机构
[1] M3 Engn & Technol, 2051 W Sunset Rd,Suite 101, Tucson, AZ 85704 USA
[2] Natl Solar Observ, Tucson, AZ 85719 USA
来源
ADAPTIVE OPTICS SYSTEMS III | 2012年 / 8447卷
关键词
solar astronomy; adaptive optics; wavefront correction; PID control; automatic tuning;
D O I
10.1117/12.927169
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We present the study and results on automatic tuning and optimizing the closed-loop control gains of the Proportional Integral (PI) controller for the high-order adaptive optics (HOAO) system. The Ziegler-Nichols frequency response (ZNfr) method is examined using the Nyquist stability criterion to implement the automatic tuning of PI controller by determining the ultimate gain, K-u, and ultimate period, T-u, of a process model, which consists of components from adaptive optics (AO) system. The maximum magnitude criterion, 0.5 <= dB <= 2.3, is identified and considered as the optimization method, which also established the stability of the PI controller. MATLAB scripts are developed to execute iterative calculation of control algorithm, which automates real-time simulation of the Simulink high-order adaptive optics (Sim-HOAO) models. Simulink block diagrams are used to represent transfer functions, which described the frequency-domain behavior of the AO system.
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页数:13
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