首页> 外文会议>Conference on Optical Modeling and Performance Predictions >Optical performance analysis and optimization of large telescope structural designs
【24h】

Optical performance analysis and optimization of large telescope structural designs

机译:大望远镜结构设计的光学性能分析与优化

获取原文

摘要

We describe a tool to analyze the effects of gravity induced deflections on a telescope structure with segmented primary mirror optics. An objective of the telescope structural design process is to minimize image quality degradation due to uncorrectable static deflections of the optics under gravity, while ensuring that the overall system meets several requirements including limits of maximum primary mirror actuator stroke, segment rotation and decenter, and secondary mirror actuation. These design and performance criteria are not readily calculated within a finite element program. Our Merit Function routine, implemented in MATLAB and called by ANSYS, calculates these parameters and makes them available within ANSYS for evaluation and design optimization. In this analysis, ANSYS outputs key structural-model nodal displacements to a file, which are used to determine the 6 degree of freedom motion of the telescope's optical surfaces. MATLAB then utilizes these displacements, along with a database containing coordinate system transforms and a linear optics model derived from ZEMAX, to calculate various performance criteria. The values returned to ANSYS can be used to iteratively optimize performance over a set of structural design parameters. Optical parameters calculated by this routine include the optical path difference at the pupil, RMS wavefront, encircled energy and low order Zernike terms resulting from primary mirror segment rotation and decenter. Also reported are the maximum actuator strokes required to restore tip-tilt and piston of the primary mirror segments, and the deflection of the secondary mirror under gravitational load. The merit function routine is being used by the Thirty Meter Telescope (TMT) project to optimize and assess the performance of various telescope structural designs. This paper describes the mathematical basis of the calculations, their implementation and gives preliminary results of the TMT Telescope Structure Reference Design.
机译:我们描述了一种工具,用于分析重力诱导偏转对具有分段初级镜光光学望远镜结构的效果。望远镜结构设计过程的目的是最小化由于重力下光学静态偏转而最小化的图像质量劣化,同时确保整个系统满足了几种要求,包括最大主镜式执行器行程,段旋转和偏移的限制,以及次级镜子致动。这些设计和性能标准不容易在有限元程序中计算。我们在MATLAB中实现的MESIT函数例程并由ANSYS调用,计算这些参数,并使其在ANSYS中可用以进行评估和设计优化。在该分析中,ANSYS将密钥结构模型节点位移输出到用于确定望远镜光学表面的6度的自由运动。然后,MATLAB利用这些位移,以及包含坐标系转换的数据库和从ZEMAX导出的线性光学器件模型,以计算各种性能标准。返回到ANSYS的值可用于迭代优化在一组结构设计参数上的性能。通过该例程计算的光学参数包括瞳孔的光路径,RMS波前,环绕的能量和由主镜段旋转和变得置换产生的低阶Zernike术语。还报道了恢复初级镜段的尖端倾斜和活塞所需的最大致动器笔划,以及在重力负荷下的二次镜的偏转。三十米望远镜(TMT)项目正在使用优点函数例程,优化和评估各种望远镜结构设计的性能。本文介绍了计算的数学依据,实现并提供了TMT望远镜结构参考设计的初步结果。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号