LSST Telescope Modeling Overview

被引:5
作者
Sebag, J. [1 ]
Andrew, J. [1 ]
Angeli, G. [1 ]
Araujo, C. [1 ]
Barr, J. [1 ]
Callahan, S. [1 ]
Cho, M. [1 ]
Claver, C. [1 ]
Daruich, F. [1 ]
Gressler, W. [1 ]
Hileman, E. [1 ]
Liang, M. [1 ]
Muller, G. [1 ]
Neill, D. [1 ]
Schoening, B. [1 ]
Warner, M. [1 ]
Wiecha, O. [1 ]
Xin, B. [1 ]
Orden Martinez, Alfredo [2 ]
Perezagua Aguado, Manuel [2 ]
Garcia Marchena, Luis [2 ]
Ruiz de Argandona, Ismael [3 ]
机构
[1] Large Synopt Survey Telescope, 950 N Cherry Ave, Tucson, AZ 85719 USA
[2] GHESA Ingn & Tecnol SA, Madrid, Spain
[3] IK4 Tekniker Res Alliance, Gipuzkoa, Spain
来源
MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY VII | 2016年 / 9911卷
关键词
LSST; telescope; modeling; FEM;
D O I
10.1117/12.2233178
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During this early stage of construction of the Large Synoptic Survey Telescope (LSST), modeling has become a crucial system engineering process to ensure that the final detailed design of all the sub-systems that compose the telescope meet requirements and interfaces. Modeling includes multiple tools and types of analyses that are performed to address specific technical issues. Three-dimensional (3D) Computer aided Design (CAD) modeling has become central for controlling interfaces between subsystems and identifying potential interferences. The LSST Telescope dynamic requirements are challenging because of the nature of the LSST survey which requires a high cadence of rapid slews and short settling times. The combination of finite element methods (FEM), coupled with control system dynamic analysis, provides a method to validate these specifications. An overview of these modeling activities is reported in this paper including specific cases that illustrate its impact.
引用
收藏
页数:9
相关论文
共 9 条
[1]  
Angeli G. Z., 2016, P SPIE IN PRESS, V9911
[2]  
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