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Control System Modeling for the Thirty Meter Telescope Primary Mirror

机译:三十米望远镜主镜控制系统建模

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The Thirty Meter Telescope primary mirror is composed of 492 segments that are controlled to high precision in the presence of wind and vibration disturbances, despite the interaction with structural dynamics. The higher bandwidth and larger number of segments compared with the Keck telescopes requires greater attention to modeling to ensure success. We focus here on the development and validation of a, suite of quasi-static and dynamic modeling tools required to support the design process, including robustness verification, performance estimation, and requirements flowdown. Models are used to predict the dynamic response due to wind and vibration disturbances, estimate achievable bandwidth in the presence of control-structure-interactiori (CSI) and uncertainty in the interaction matrix, and simulate and analyze control algorithms and strategies, e.g. for control of focus-mode, and sensor calibration. Representative results illustrate TMT performance scaling with parameters, but the emphasis is on the modeling framework itself.
机译:三十米望远镜的主镜由492个部分组成,尽管存在结构和动力学的相互作用,但在存在风和振动干扰的情况下,这些部分仍可进行高精度控制。与凯克望远镜相比,更高的带宽和更大的段数需要更加注意建模以确保成功。我们在这里专注于支持设计过程所需的一套准静态和动态建模工具的开发和验证,其中包括鲁棒性验证,性能估计和需求缩减。使用模型来预测由于风和振动扰动引起的动态响应,在存在控制结构交互作用(CSI)和交互矩阵存在不确定性的情况下估计可实现的带宽,并模拟和分析控制算法和策略,例如用于控制聚焦模式和传感器校准。代表性的结果说明了使用参数进行TMT性能缩放,但是重点在于建模框架本身。

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