FAST进给舱新型冗余结构的解析优化方法

Jianing Yin, R. Yao, P. Jiang
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引用次数: 0

摘要

500米口径球面射电望远镜(FAST)是世界上最大的单碟射电望远镜,也是最灵敏的射电望远镜。随着观测任务数量和难度的逐年增加,决定进一步提高FAST的性能。为此,设计了一种新的FAST进给舱冗余结构。本文讨论了这种冗余构型的建模和两种约束的解析优化方法。经过仿真计算,得到了较好的优化结果。证明观测天顶角至少可以达到50°,这意味着可以观测到银河系中心附近的天文现象。研究结果为FAST的未来升级提供了重要依据。
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Analytical Optimization Method for the New Redundant Configuration of the FAST Feed Cabin
The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is the largest single dish and most sensitive radio telescope in the world. As the number and difficulty of observation tasks increase year by year, it is decided to further improve the performance of FAST. Therefore, a new redundant configuration of the FAST feed cabin has been designed. This paper discusses the modeling of such redundant configuration and the analytical optimization method with 2 kinds of constrains. Then after simulation calculation, an excellent optimization result is obtained. It proves that at least 50° observation zenith angle can be achieved, which means that astronomical phenomena near the galactic center can be observed. The results provide the important foundation for the FAST’s future upgrade.
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