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地基激光测距系统观测空间碎片进展
引用本文:张海峰,邓华荣,吴志波,汤凯,张忠萍. 地基激光测距系统观测空间碎片进展[J]. 航天器环境工程, 2016, 33(5): 457-462
作者姓名:张海峰  邓华荣  吴志波  汤凯  张忠萍
作者单位:1. 中国科学院 上海天文台, 上海 200030;2. 中国科学院 空间目标与碎片观测重点实验室, 南京 210008
基金项目:国家自然科学基金项目(编号:11303074,11503068);中国科学院国防创新基金项目(编号:CXJJ-14-S108);中国科学院重大装备项目(编号:2920100701);国家国防科工局空间碎片“十二五”预先研究项目(编号:K0103110)
摘    要:卫星激光测距作为地基光电望远镜系统重要技术应用,可直接精确测量空间碎片距离,提升碎片目标轨道监测精度。基于上海天文台60 cm口径激光测距望远镜,应用百赫兹重复率高功率激光器、高效率激光信号探测系统等,建立了空间碎片激光测距系统,实现了对距离500~2600 km、截面积0.3~20 m2的碎片目标观测,测距精度优于1 m,具备了碎片目标常规测量与应用能力。此外,开展了空间目标白天监视技术研究,实现了亮于6星等恒星的白天观测,并进行了望远镜局部指向误差模型分析,分析结果可应用于空间碎片白天激光观测的目标监视与引导。

关 键 词:空间碎片  激光测距  观测系统  白天恒星监视
收稿时间:2016-07-29
修稿时间:2016-08-29

Observations of space debris by ground-based laser ranging system
ZHANG Haifeng,DENG Huarong,WU Zhibo,TANG Kai,ZHANG Zhongping. Observations of space debris by ground-based laser ranging system[J]. Spacecraft Environment Engineering, 2016, 33(5): 457-462
Authors:ZHANG Haifeng  DENG Huarong  WU Zhibo  TANG Kai  ZHANG Zhongping
Affiliation:1. Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;2. Key Laboratory of Space Object and Debris Observation, Chinese Academy of Sciences, Nanjing 210008, China
Abstract:The satellite laser ranging is one of the important application technologies for the ground-based optical-electronic telescope system, and the distance of the space debris is directly measured to improve the orbit accuracy. Based on the laser ranging telescope with the aperture of 60cm at the Shanghai Astronomical Observatory, the space debris laser ranging system is set up with the development of a high power laser system of hundreds hertz repetition rate and a laser signal detection system of high efficiency. The routine laser observation of space debris may be realized with the measured distance from 500 km to 2600 km, the cross section from 0.3 m2 to 20 m2, the ranging precision of better than 1 m, for accurately measuring the space debris. In addition, the method of monitoring the space targets in the daytime is also studied preliminarily, and the stars brighter than six magnitude of brightness are observed to make the regional pointing error correction model. The method can be applied in the monitoring and guiding for the daylight space debris laser ranging.
Keywords:space debris  laser ranging  observing system  daylight star guiding
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