Structure of distributed control system in Seimei telescope

被引:1
作者
Jikuya I. [1 ]
Uchida D. [2 ]
Kino M. [3 ]
Kurita M. [4 ]
Yamada K. [5 ]
机构
[1] Institute of Science and Engineering, Kanazawa University, Kanazawa
[2] Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa
[3] Astronomical Observatory, Kyoto University, Kyoto
[4] Department of Astronomy, Kyoto University, Kyoto
[5] Department of Mechanical Engineering, Osaka University, Suita, Osaka
基金
日本学术振兴会;
关键词
distributed control; large system; Position control; segmented mirror; telescope;
D O I
10.1080/18824889.2021.1913879
中图分类号
学科分类号
摘要
A segmented mirror control system is indispensable for operating an astronomical telescope which is equipped with a segmented primary mirror. In this study, we focus on the distributed control system (DCS) proposed for Seimei telescope. An interesting hierarchical structure is found by analysing its zero–nonzero structure in the DCS, and then, 54 gains are reasonably classified into 4 groups. Design examples for selecting gains of the DCS are presented so that the closed loop pole locations are similar to those of the centralized control system (CCS). The freedom in the selections of gains by taking account of the hierarchical structure is shown to be effective by numerically evaluating the stability region and by optimizing the maximum distance between the closed loop poles of DCS and CCS. © 2021 The Author(s). Published by Informa UK Limited, trading as Taylor & Francis Group.
引用
收藏
页码:111 / 118
页数:7
相关论文
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