一种空间目标可见光反射特性控制技术

黄晨; 王建军; 薛莉; 高昕; 宋平

doi:10.13700/j.bh.1001-5965.2014.0422

一种空间目标可见光反射特性控制技术

doi: 10.13700/j.bh.1001-5965.2014.0422

黄晨^1, ,,
王建军¹,
薛莉¹,
高昕¹,
宋平²

1.
北京跟踪与通信技术研究所, 北京 100094
2. 西安卫星测控中心, 西安 710049

详细信息

通讯作者:
黄晨(1987—),男,福建尤溪人,助理研究员,raulhuang2010@gmail.com,研究方向为光学特性测量、图像处理.

中图分类号: V557.4
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出版历程
- 收稿日期: 2014-07-16
- 网络出版日期: 2015-06-20

New control technology for visible light reflection characteristics of space target

1.
Beijing Institute of Tracking and Telecommunications Technology, Beijing 100094, China
2. Xi'an Satellite Control Center, Xi'an 710049, China

摘要

摘要: 目前对于地球同步轨道(GEO)空间目标的探测和识别主要依靠反射太阳光的光度变化进行分析识别并判断.基于空间目标表面漫反射性质的可见光反射特性计算模型分析,研究了不同形状反射体可见光反射特性,并提出一种采用不同形状反射体控制改变空间目标可见光反射特性的方法.以GEO卫星为例,采用基于蒙特卡罗的非序列光线追迹方法,仿真分析椎体、球体和圆柱体作为反射控制体对卫星光变特性的影响.结果表明该方法可改变卫星原有可见光反射光变曲线,降低卫星被探测识别概率,提高空间目标隐蔽性.
- 空间目标 /
- 光变曲线 /
- 可见光反射特性 /
- 反射控制体 /
- 卫星可见光隐身
Abstract: For geosynchronous (GEO) orbit space object's detection and recognition is mainly dependent on analysis, identification and judgment of reflected sunlight photometric curve. Based on analysis of visible light reflection characteristics calculation model of space target surface diffuse reflection properties, a study on different shape reflector light reflection characteristics was carried out. Moreover, a different shape reflector method was proposed to control space target light reflection characteristics. Taking an example of a GEO satellite, simulate and analyze the effects of cone, sphere and cylinder as reflection control body on satellite reflection characteristics by using Monte Carlo non-sequential light tracing method. The results show that the method can change the satellite original visible light reflection curve, reduce the probability of being detected and recognized, and improve the invisibility of space object.
- space object /
- light curve /
- visible light reflection characteristics /
- reflection control body /
- satellite visible light stealth

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参考文献(15)

[1]	Oswald M, Krag H, Wegener P, et al.Concepts for an orbital telescope observing the debris environment in GEO[J].Advances in Space Research, 2004, 34(5):1155-1159.
[2]	Matney M J, Stansbery E, Africano J, et al.Extracting GEO orbit populations from optical surveys[J].Advances in Space Research, 2004, 34(5):1160-1165.
[3]	Isobe S, Asami A, Asher D, et al.A new 1M telescope for space debris survey observations[J].Advances in Space Research, 2004, 34(5):917-920.
[4]	Seitzer P, Smith R, Africano J, et al.MODEST observations of space debris at geosynchronous orbit[J].Advances in Space Research, 2004, 34(5):1139-1142.
[5]	Schildknecht T, Musci R, Ploner M, et al.Optical observations of space debris in GEO and in high-eccentric orbits[J].Advances in Space Research, 2004, 34(5):901-911.
[6]	Rudenko S P, Tarady V K, Sergeev A V, et al.Determination of orbit of geosynchronous space debris Kupon satellite using its CCD observations at 2-meter telescope at Terskol peak[C]//Dynamics of Natural and Artificial Celestial Bodies.Berlin:Springer, 2001, 8:373-374.
[7]	唐轶峻, 姜晓军, 魏建彦, 等.高轨空间碎片光电观测技术综述[J].宇航学报, 2008, 29(4):1094-1098. Tang Y J, Jiang X J, Wei J Y, et al.Review of optical observations of high apogee space debris[J].Journal of Astronautics, 2008, 29(4):1095-1097(in Chinese).
[8]	陈荣利, 韩乐, 车驰骋, 等.非自发光空间目标的可见光探测技术研究[J].光子学报, 2005, 34(9):1438-1440. Chen R L, Han L, Che C C, et al.Research on un-illuminant space target visual detection technique[J].Acta Photonica Sinica, 2005, 34(9):1438-1440(in Chinese).
[9]	刘云猛, 柴金广, 王旭辉, 等.空间目标可见光特性与探测距离估算[J].红外技术, 2009, 31(1):23-26. Liu Y M, Chai J G, Wang X H, et al.Visible characteristics and calculation of detecting distance for space target[J].Infrared Technology, 2009, 31(1):23-26(in Chinese).
[10]	Sridharan R, Burnham B, et al.Performance improvements of the SBV[C]//Proceedings of the Space Control Conference.Lexington, Massachusetts:Massachusetts Institute of Technology Lincoln Laboratory, 1998:71-80.
[11]	Africano J L, Stansbery E G, Kervin P W.The optical orbital debris measurement program at NASA and AMOS[J].Advances in Space Research, 2004, 34(5):892-900.
[12]	Stokes G H, von Braun C, Sridharan R, et, al.The space-based visible program[J].Lincoln Laboratory Journal, 1998, 11(2):205-238.
[13]	庄诚.基于太阳赤纬角的地球同步轨道(GEO)空间碎片光度测量标定方法的研究[D].杭州:浙江工业大学, 2011. Zhuang C.The research of photometric calibration of geosynchronous orbit (GEO) space debris under solar declination[D].Hangzhou:Zhejiang University of Technology, 2011(in Chinese).
[14]	Nayar S K, Ikeuchi K, Kanade T.Determining shape and reflectance of hybrid surfaces by photometric sampling[J].Robotics and Automation, IEEE Transactions on, 1990, 6(4):418-431.
[15]	李斌成.空间目标的光学特性分析[J].光电工程, 1989(2): 21-26. Li B C.Optical characteristic analysis of space target[J].Opto-Electronic Engineering, 1989(2):21-26(in Chinese).