摘要
500 m口径球面射电望远镜(Five-hundred-meter Aperture Spherical Radio Telescope,FAST)的跟踪观测需要馈源的空间运动配合,馈源舱主要用于实现馈源的精调定位,因此馈源舱位置的高精度测量对FAST望远镜的高效运行意义重大。但当全站仪设备失效时,无法对采用Kalman算法的GPS/IMU融合测量结果进行修正,导致馈源舱测量精度下降。为了解决这个问题,设计了基于BP(back propagation)神经网络的预测模型,包括数据预处理、模型设计和模型训练验证。模型训练数据为FAST真实测量数据,数据量为40 GB左右。为了验证模型的泛化能力,选取三种运动轨迹数据对模型预测精度进行测试,结果显示,三种运动轨迹下精度都满足15 mm要求。
When the Five-hundred-meter Aperture Spherical Radio Telescope(FAST)performs the tracking observation task,for cooperating with this task,the feed has got spatial motion.The fine-tuning positioning of the feed is realized by the feed cabin,so the highprecision measurement of the position of the feed cabin is great significance.However,when the total station equipment fails,it is unable to correct the GPS/IMU fusion measurements with the Kalman algorithm,it causes the accuracy of the feed cabin measurements decreasing.In order to solve this problem,this paper designs a prediction model based on BP neural network,which is composed of three parts,the data preprocessing,the model design and the model training validation.And the model training data is the real measurement data of FAST with a data volume of about 40 GB.In order to verify the generalization ability of the model,three kinds of motion trajectory data are selected to test the model prediction accuracy,and the results show that the accuracy meets the 15 mm requirement under three kinds of motion trajectories.
作者
卢朝茂
李明辉
宋本宁
彭帅
冯禹
于东俊
骆亚波
LU Chao-mao;LI Ming-hui;SONG Ben-ning;PENG Shuai;FENG Yu;YU Dong-jun;LUO Ya-bo(State Key Laboratory of Public Big Data,Guizhou University,Guiyang 550025,China;Na-tional Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;Changsha University of Science and Technology,Changsha 410114,China)
出处
《天文学进展》
CSCD
北大核心
2024年第3期519-528,共10页
Progress In Astronomy
基金
国家自然科学基金(12363010,42274055)
贵州省科技计划项目(黔科合基础-ZK[2023]一般039,黔科合支撑[2023]一般352)。