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基于快反镜提高激光测距回波率的方法研究
其他题名Research on Improving the Laser Ranging Echo Rate Based on FSM
李鹏飞
学位类型博士
导师李祝莲
2023
学位授予单位中国科学院大学
学位授予地点北京
学位专业天体测量与天体力学
关键词空间目标激光测距 快反镜 速度光行差 测距回波率 闭环控制
摘要激光测距是目前空间目标距离测量中,测量精度较高的一种技术,测量数据具有非常重要的科学研究和应用价值。云南天文台1.2m望远镜开展激光测距研究和试验多年,目前已具备开展卫星、空间碎片以及月面反射器等空间目标激光测距的能力。使用1.2m望远镜测距系统,研究团队于2017年测到了36cm直径分米级尺寸空间碎片的距离,2018年初测到了月面反射器的距离,可见该系统具有较好的探测性能。为了进一步开发1.2m望远镜测距系统的探测能力,本论文研究提高测距系统回波率的新方法,主要完成工作如下: 第一,根据1.2m望远镜测距技术现状和难瞄准的问题,提出一种提高测距系统回波率的方法,即利用快反镜的快速响应、分辨率高等特点来确保空间目标的高精度跟瞄,从而提高测距系统回波率。1.2m望远镜测距系统虽然已具备了较好的探测性能,但是依然存在一些细节问题需要解决,进一步提高回波率后,系统将具备深空合作目标以及更小尺寸、更远距离非合作目标的激光测距能力。 第二,分析了激光测距中影响回波率的因素,包括速度光行差、望远镜跟踪误差、大气湍流和望远镜指向偏差等。得出速度光行差随目标轨道高度的变化关系,空间目标的最大速度光行差随轨道高度增大而减小,低轨目标的最大速度光行差有 10′′ 左右,而月面反射器的最大速度光行差只有 1.4′′,利用快反镜可以对空间目标的较小偏离进行修正。 第三,将快反镜应用于1.2m望远镜发射光路中,利用快反镜高分辨率高精度控制激光光束方向,达到提高测距成功率和回波光子数的目的。首先,分析了快反镜在发射光路的位置排布设计;然后,测试了发射光路带有快反镜后系统的分辨率并开展系统模拟仿真;最后,跟踪卫星进行快反镜开环控制试验。结果表明,快反镜可以在激光测距中用搜索的方式找到回波更强的位置,且目标距离越远效果越明显。 第四,提出使用回波数作为快反镜闭环控制反馈量的新快反镜控制算法,并取得了较好的控制效果。设计了快反镜闭环控制系统,并在1.2m望远镜高精度指向的基础上对不同轨道高度的卫星开展了闭环控制试验。结果表明,使用快反镜闭环控制后,在不同的观测条件下,回波率都得到了提高。 第五,仿真分析了将快反镜应用于1.2m望远镜激光测距系统的可行性。首先,设计快反镜在接收光路的位置排布;然后,计算了接收光路中视场光阑孔径对接收视场的影响,并开展卫星测距试验以统计不同目标的回波信号在接收视场中的分布情况;最后仿真了快反镜在回波信号不同偏离角度时的校正能力。 综上所述,本论文将高速高分辨率的快反镜应用于1.2m望远镜激光测距系统,通过提高系统测距回波率来达到提高系统探测能力的目的,对白天空间目标激光测距、月球激光测距以及更远的深空激光测距具有一定的参考价值。
其他摘要Laser ranging is a technology with high measurement accuracy in the range measurements of space targets at present. The measured data has very important scientific research and application value. The 1.2m telescope of Yunnan Observatories has carried out laser ranging research and test for many years, and now has the ability to carry out laser ranging for space targets such as satellites, space debris and lunar reflectors. Using the 1.2m telescope laser ranging system, the research team measured the distance of space debris with a 36cm diameter in 2017, and the distance of the lunar retroreflector in early 2018, which shows that the system has good detection capability. In order to further develop the detection capability of the 1.2m telescope ranging system, this paper studies a new method to improve the echo rate of the ranging system. The main work is as follows: First, according to the current situation and existing problems of the ranging technology of 1.2m telescope, a method to improve the echo rate of the ranging system is proposed, that is, the quick response and high resolution FSM are used to ensure the high-precision tracking and aiming of space targets, so as to improve the echo rate of the ranging system. Although the 1.2m telescope ranging system has good detection performance, there are still some details to be solved. After further improving the echo rate, the system will have the laser ranging capability for deep space cooperative targets and smaller, more distant non cooperative targets. Secondly, the factors that affect the echo rate in laser ranging are analyzed, including velocity aberration, telescope tracking error, atmospheric turbulence and telescope pointing error.And the relationship between velocity aberration and target orbital height is obtained. The maximum velocity aberration of space target decreases with the increase of orbital height.The maximum velocity aberration of the LEO target is about 10 ", while the maximum velocity aberration of the lunar reflector is only 1.4". The small deviation of the space target can be corrected by FSM. Thirdly, the FSM is applied to the transmission optical path of 1.2m telescope, and the FSM is used to control the laser beam direction with high resolution and high precision, so as to improve the success rate of laser ranging and the number of returned photons. (1) Analyzing the the position of FSM in transmitting optical path; (2)The resolution of the system with FSM in the transmitting optical path is tested and the effect of FSM in transmitting optical path is simulated;(3)The experiment is carried out for the FSM open-loop control by observing satellites. The experimental results show that the FSM can find the position with stronger echo by searching in laser ranging, and the farther the target is, the more obvious the effect is. Fourthly, a new FSM control algorithm is proposed, which uses the echo photon number as the feedback value of the FSM closed-loop control, and achieves good control effect. The closed-loop control system of the FSM is designed, and the closed-loop control tests are carried out for satellites with different orbital heights on the basis of the high-precision pointing of the 1.2m telescope. The test results show that the echo rate is improved under different observation conditions after using FSM closed-loop control. Fifthly, the feasibility of applying FSM to the 1.2m telescope laser ranging system is simulated and analyzed. First, the position of the FSM in the receiving optical path is designed; Then, the influence of the diameter of aperture in the receiving optical path on the receiving field view is calculated, and the satellite ranging test is carried out to calculate the distribution of echo signals of different targets in the receiving field view; Finally, the correction ability of FSM at different deviation angles of the echo signal is simulated. To sum up, this paper applies the high-speed and high-resolution FSM to the 1.2m telescope laser ranging system, and improves the system's detection capability by improving the system's ranging echo rate. It has certain reference value for daytime space target laser ranging, lunar laser ranging, and further deep space optical ranging.
学科领域天文学
学科门类理学 ; 理学::天文学
页数0
语种中文
文献类型学位论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/26415
专题应用天文研究组
作者单位中国科学院云南天文台
第一作者单位中国科学院云南天文台
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李鹏飞. 基于快反镜提高激光测距回波率的方法研究[D]. 北京. 中国科学院大学,2023.
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