Detecting performance and overall design of airborne daytime star sensor for navigation

ZHONG Xing; JIAO Ji-qiang; JIN Guang; QU Hong-song; LIU Guo-song

doi:10.3788/OPE.20111912.2900

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Detecting performance and overall design of airborne daytime star sensor for navigation

Article | 更新时间：2020-08-12

- Detecting performance and overall design of airborne daytime star sensor for navigation
- Optics and Precision Engineering Vol. 19, Issue 12, Pages: 2900-2906(2011)
- 作者机构：
  
  中国科学院长春光学精密机械与物理研究所,吉林长春,中国,130033
- 作者简介：
- 基金信息：
- DOI：10.3788/OPE.20111912.2900
  CLC： V448.22
- Received：18 February 2011，
  
  Revised：25 May 2011，
  
  Published Online：25 December 2011，
  
  Published：25 December 2011
- 稿件说明：
移动端阅览
钟兴, 贾继强, 金光, 曲宏松, 刘国嵩. 机载导航白天星敏感器的探测性能及总体设计[J]. 光学精密工程, 2011,19(12): 2900-2906

ZHONG Xing, JIAO Ji-qiang, JIN Guang, QU Hong-song, LIU Guo-song. Detecting performance and overall design of airborne daytime star sensor for navigation[J]. Editorial Office of Optics and Precision Engineering, 2011,19(12): 2900-2906
钟兴, 贾继强, 金光, 曲宏松, 刘国嵩. 机载导航白天星敏感器的探测性能及总体设计[J]. 光学精密工程, 2011,19(12): 2900-2906 DOI： 10.3788/OPE.20111912.2900.

ZHONG Xing, JIAO Ji-qiang, JIN Guang, QU Hong-song, LIU Guo-song. Detecting performance and overall design of airborne daytime star sensor for navigation[J]. Editorial Office of Optics and Precision Engineering, 2011,19(12): 2900-2906 DOI： 10.3788/OPE.20111912.2900.

摘要

理论分析和试验研究了机载导航白天星敏感器的探测性能

建立了白天观星的信噪比和调制度在噪声影响下的数学模型

对比了焦距一定

不同入瞳直径和入瞳直径一定

不同焦距情况下的计算结果。归纳了光学系统的性能要求及系统参数对探测效果的影响

得出光学系统相对孔径为1/15较为合适的结论。在此基础上提出了用于3等星全天时观测的白天星敏原理样机的光机及电子学处理总体方案。利用相对孔径为1/15的望远物镜进行地面实验

获得了对北极星从日出到正午的持续观测结果。对比不同时刻星点图像的亮度和对比度变化显示

随着太阳高度角增大

星点图像的对比度由上午5:00的1.55下降到正午12:00的1.2左右

据此换算出样机方案的探测性能指标。计算结果表明

采用口径为

70 mm

相对孔径为1/15的光学系统可满足对3等星的探测最小调制度为0.03的要求。实验表明

本文进行的理论分析正确

方案合理可行

可为小型高精度机载导航星敏感器的研制提供参考。

Abstract

The detecting performance of an airborne daytime star sensor for navigation is analyzed and a daytime star sensor prototype is researched. Mathematical models of Signal to Noise-Ratio(SNR) and contrast of a photoelectric imaging system in daytime under noises are established

and calculated results by different focal lengths and different apertures are compared to conclude the influence of system parameters on the detection results and the requirements of optical system.The conclusion shows that the proper relative aperture of optical system is 1/15. A daytime star sensor prototype for tracking stars of magnitude 3 is designed. Tracking images of the polestar from sunrise to noon are acquired by a ground experiment using a

/15 objective

and brightnesses and contrasts of star images at different time are compared. It shows that the contrast of star image has descended from 1.55 at 5:00 a.m. to 1.2 at 12:00 a.m. The minimal degree of modulation is more than 0.03 by calculating with the prototype's parameters

which shows that the optical system with

70 mm and

/15 can satisfy the detecting requirements. The theoretic analysis and design is proved to be available

and the research can be a reference for developing of miniaturized and precise airborne daytime navigation star sensors.

关键词

Keywords

references

DUNCAN T M. A daylight stellar sensor using a charge-coupled device[J]. SPIE,1989,1111:1-14.[2] DIETZ K L,RAMSEY B D. Daytime aspect camera for balloon altitudes[J]. Opt. Eng., 2002,41(10):2641-2651.[3] SANDVEN S C,BROWNE S L. Tip-tilt tracker for image stabilization in a daylight speckle imaging system [J]. SPIE, 1995,2468: 246-251.[4] 沈湘衡,李清军,王建军. 利用视频判读进行白天测星方法的研究[J]. 光学精密工程,2000,8(2):189-191. SHEN X H, LI Q J, WANG J J. Measuring star with video interpretation in daytime[J]. Opt. Precision Eng., 2000,8(2):189-191.(in Chinese)[5] 张双同,李清军,沈湘衡. 提高海上白天测星能力的方法研究[J]. 光学精密工程,2000,8(3):261-264. ZHANG SH T,LI Q J,SHEN X H. Method of measuring star at sea in daytime[J]. Opt. Precision Eng., 2000,8(3): 261-264.(in Chinese)[6] 王伟国.空间目标白天光电探测技术研究. 北京:中国科学院研究生院博士学位论文,2005. WANG W G. Research of space object detecting under bright background. Beijing:Doctor Degree Dissertation of Graduate School of the Chinese Academy of Sciences,2005.(in Chinese)[7] 徐维安. 光谱滤波装置在白天测星中的应用[J]. 光学精密工程,1996,4(4):84-88. XU W A. Application of spectral filter device in measuring stellar in daytime[J]. Opt. Precision Eng., 1996, 4(4):202-206.(in Chinese)[8] 张己化,姚东升,谈斌. 地基光电系统空间目标探测影响因素分析[J]. 光学学报,2008,28(6):1178-1182. ZHANG J H,YAO D SH,TAN B. Analysis on effect factors of ground based electro-optic system detection ability on space object [J]. Acta Optica Sinica, 2008,28(6):1178-1182.(in Chinese)[9] 王建军. 白天强天空背景条件下空间目标探测能力分析[J]. 飞行器测控学报,2007,26(6):45-49. WANG J J. An analysis of detection capability to space object in daytime strong sky background [J]. Journal of Spacecraft TT&C Technology, 2007,26(6):45-49.(in Chinese)[10] 王晶, 高利民,姚俊峰. 机载测量平台中的坐标转换误差分析[J]. 光学精密工程, 2009, 17(2):388-394. WANG J,GAO L M,YAO J F. Analysis on coordinate conversion error of airborne measuring device [J]. Opt.Precision Eng., 2009, 17(2):388-394.(in Chinese)[11] 耿文豹, 翟林培, 丁亚林. 振动对光学成像系统传递函数影响的分析[J]. 光学精密工程, 2009, 17(2):314-320. GENG W B,ZHAI L P,DING Y L. Analysis of influence of vibration on transfer function in optics imaging system [J]. Opt. Precision Eng., 2009, 17(2):314-320.(in Chinese)[12] 李欣,赵亦工, 陈冰,等. 基于模糊分类的弱小目标检测方法[J]. 光学精密工程, 2009, 17(9):2311-2320. LI X, ZHAO Y G,CHEN B,et al. Approach to dim and small target detection based on fuzzy classification [J]. Opt. Precision Eng., 2009, 17(9):2311-2320.(in Chinese)[13] 管志强,陈钱,钱惟贤,等. 一种背景自适应调整的弱点目标探测算法[J]. 光学学报, 2007, 27(12): 2163-2168. GUAN ZH Q,CHEN Q,QIAN W X,et al. An adaptive background adjusting algorithm for dim target detection [J]. Acta Optica Sinica, 2007, 27(12):2163-2168.(in Chinese)[14] 尚海林. 复杂场景下弱小目标检测算法的FPGA实现[J]. 航空兵器, 2007(4):22-24. SHANG H L. A detection algorithm of small targets in complex background implemented by FPGA [J]. Aero Weaponry, 2007(4):22-24.(in Chinese)[15] 冯小勇,朱明,向治强. 白天暗小恒星目标电视实时探测[J]. 光学学报,2010, 30(4):1009-1014. FENG X Y,ZHU M,XIANG ZH Q. Method of television real-time detection on dark and small stars targets in the daytime [J]. Acta Optica Sinica, 2010, 30(4):1009-1014.(in Chinese)

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