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Model order reduction and controller design for segmented primary mirror of a large optical telescope.

机译:大型光学望远镜分段主镜的模型降阶和控制器设计。

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摘要

The Very Large Optical Telescope (VLOT) is a concept, proposed by the National Research Council - Herzberg Institute of Astrophysics, to address future demands of the international astrophysics community. To develop and evaluate the VLOT designs, an Integrated Modeling approach is employed. The Integrated Model (IM) is a single simulation tool which accounts for the interactions between different telescope modules to produce the final image quality generated by the telescope. The work in this thesis relates directly to two of the modules of the IM: (1) the structural dynamics and (2) the primary mirror control module.; In order to obtain accurate optical performance predictions from the IM, a high fidelity structural model of the telescope is required. However, the finite-element model of the telescope, which is its nascent structural model, is prohibitively large in size for practical simulation. This problem can be addressed by applying a suitable Model Order Reduction technique. In the first half of this thesis, we compare five Model Order Reduction techniques from the literature for the VLOT application. These methods are evaluated and compared in frequency and time domains. Based on these results, we conclude that the Singular Perturbation Approximation method is suitable for the VLOT application.; The primary mirror, which is the main light-gathering surface of the telescope, must be maintained in a particular profile in order to provide the desired image quality. Currently, this control objective is achieved with an enhanced integral controller based on a SISO control approach. The primary mirror, however, is a MIMO system and hence the second objective of this thesis is to evaluate a MIMO control design approach, in particular, the Linear Quadratic Gaussian (LQG) controller. The LQG design is evaluated in two steps: initially with a single mirror segment model and then with the VLOT structural model. Based on our results, we conclude that even with currently available computational resources, it is not feasible to employ the LQG control approach in a centralized manner to a large scale system such as VLOT.
机译:超大型光学望远镜(VLOT)是由美国国家研究委员会-赫兹伯格天体物理学研究所提出的一种概念,用于解决国际天体物理学界的未来需求。为了开发和评估VLOT设计,采用了集成建模方法。集成模型(IM)是一个单一的仿真工具,用于说明不同望远镜模块之间的相互作用,以产生由望远镜生成的最终图像质量。本文的工作直接与IM的两个模块有关:(1)结构动力学和(2)主镜控制模块。为了从IM获得准确的光学性能预测,需要望远镜的高保真结构模型。但是,望远镜的有限元模型(它的新生结构模型)在实际模拟中尺寸过大。可以通过应用适当的模型降阶技术来解决此问题。在本文的上半部分,我们比较了文献中针对VLOT应用的五种模型降阶技术。对这些方法进行了评估,并在频域和时域进行了比较。根据这些结果,我们得出结论,奇异摄动近似法适用于VLOT应用。主镜是望远镜的主要聚光表面,必须保持特定的轮廓,以提供所需的图像质量。当前,该控制目标是通过基于SISO控制方法的增强型积分控制器来实现的。然而,主反射镜是MIMO系统,因此本论文的第二个目标是评估MIMO控制设计方法,尤其是线性二次高斯(LQG)控制器。 LQG设计分两个步骤进行评估:首先使用单个镜像段模型,然后使用VLOT结构模型。根据我们的结果,我们得出结论,即使有当前可用的计算资源,将LQG控制方法以集中方式应用于大型系统(例如VLOT)也是不可行的。

著录项

  • 作者

    Yu, Kintak Raymond.;

  • 作者单位

    McGill University (Canada).;

  • 授予单位 McGill University (Canada).;
  • 学科 Engineering Mechanical.
  • 学位 M.Eng.
  • 年度 2006
  • 页码 108 p.
  • 总页数 108
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 机械、仪表工业;
  • 关键词

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