地球同步轨道暗弱目标地基光学成像技术综述
Review of ground-based optical imaging techniques for dim GEO objects
查看参考文献89篇
|
文摘
|
地基光学成像是对空间目标进行探测识别的重要手段。本文分析了近十几年间建立的用于天文观测的巨型望远镜设备不能对地球同步轨道(Geostationary Earth Orbit,GEO)目标进行高分辨率观测的主要原因:除大气湍流对成像质量的影响和分辨率的限制外,还有GEO目标尺寸和目标亮度昏暗问题。因此需要引入非传统成像技术解决上述问题。本文研究了几种采用激光照明的非传统光学成像方法,具体分析论证了稀疏孔径成像、强度相关成像、剪切光束成像和傅立叶望远术等光学成像技术,阐述了各成像技术的优势与局限性,分析了几种方法对GEO暗弱目标高分辨率成像的应用前景。 |
|
其他语种文摘
|
Ground-based optical imaging is an important method for detecting and identifying space objects.The main reasons that the giant telescopes for astronomical observation established in the last decade cannot be used for high-resolution observation of GEO objects are analyzed.It is necessary to utilize unconventional imaging technology to solve image degradation due to GEO objects' small size,low-reflection and atmospheric turbulence.We have researched several new methods of unconventional optical imaging using laser illumination.The optical imaging techniques such as sparse aperture imaging,imaging correlography,Sheared-beam imaging and Fourier telescopy are analyzed and demonstrated.The advantages and limitations of each technique are discussed.The applications of high-resolution imaging for dim GEO objects are prospected. |
|
来源
|
中国光学
,2019,12(4):753-766 【核心库】
|
|
DOI
|
10.3788/co.20191204.0753
|
|
关键词
|
空间目标
;
高分辨率
;
光学成像技术
;
激光主动成像
|
|
地址
|
1.
中国科学院西安光学精密机械研究所, 西安, 710119
2.
中国科学院大学, 北京, 100049
|
|
语种
|
中文 |
|
文献类型
|
综述型 |
|
ISSN
|
2095-1531 |
|
学科
|
机械、仪表工业 |
|
基金
|
国家自然科学基金面上项目
|
|
文献收藏号
|
CSCD:6560268
|
参考文献 共
89
共5页
|
|
1.
王建立. 空间目标地基光电探测与识别技术的发展.
飞行器测控学报,2015,34(6):489-499
|
CSCD被引
12
次
|
|
|
|
|
2.
高扬. 中高轨道目标的地基光电监视.
光学精密工程,2017,25(10):2584-2590
|
CSCD被引
8
次
|
|
|
|
|
3.
李振伟. 暗弱空间目标的高精度定位.
光学精密工程,2015,23(9):2627-2634
|
CSCD被引
11
次
|
|
|
|
|
4.
Bakker E J. Cost estimate for the Kilometric Optical Interferometer(KOI).
Proceedings of SPIE. 7013,2008:70134F
|
CSCD被引
1
次
|
|
|
|
|
5.
Labadie L. Interferometry at the LBT.
Proceedings of Societe Francaise d'Astronomie et d' Astrophysique,SF2A,2008:73-76
|
CSCD被引
1
次
|
|
|
|
|
6.
Campbell R D. AO operations at the W. M. keck observatory.
Proceedings of SPIE. 7016,2008:701604
|
CSCD被引
1
次
|
|
|
|
|
7.
Roberts S. Optical performance analysis and optimization of large telescope structural designs.
Proceedings of SPIE. 5867,2005:58670O
|
CSCD被引
1
次
|
|
|
|
|
8.
Szeto K. TMT telescope structure system: design and development progress report.
Proceedings of SPIE. 7012,2008:70122G
|
CSCD被引
1
次
|
|
|
|
|
9.
Roberts S. Systems engineering of the thirty meter telescope through integrated opto-mechanical analysis.
Proceedings of SPIE. 7738,2010:773818
|
CSCD被引
1
次
|
|
|
|
|
10.
Murga G. Detail design and construction plans for a dome for the European Extremely Large Telescope(E-ELT).
Proceedings of SPIE. 7733,2010:773324
|
CSCD被引
1
次
|
|
|
|
|
11.
Pirnay O. Design of the unit telescopes of the MROI.
Proceedings of SPIE, 7013:70130N
|
CSCD被引
1
次
|
|
|
|
|
12.
Creech-Eakman M J. The Magdalena ridge observatory interferometer: a fully optimized aperture synthesis array for imaging.
Proceedings of SPIE. 5491,2004:405-414
|
CSCD被引
1
次
|
|
|
|
|
13.
Paresce F. Recent scientific results with the VLT interferometer.
Mem S.A.It. Suppl,2003,3:280-285
|
CSCD被引
1
次
|
|
|
|
|
14.
Benson J A. NPOI: recent technology and science.
Proceedings of SPIE. 5491,2004:464-471
|
CSCD被引
1
次
|
|
|
|
|
15.
Mcalister H A. First results from the CHARA array.I.An interferometric and spectroscopic study of the fast rotator α leonis(Regulus).
The Astrophysical Journal,2005,628(1):439-452
|
CSCD被引
2
次
|
|
|
|
|
16.
DARPA TACTICAL TECHNOLOGY OFFICE.
Broad agency announcement: Galileo,2012
|
CSCD被引
1
次
|
|
|
|
|
17.
Restaino S R. Using optical interferometry for GEO satellites imaging: an update.
Proceedings of SPIE. 9836,2016:983603
|
CSCD被引
1
次
|
|
|
|
|
18.
Office of the Director of National Intelligence.
Amon-Hen,2017
|
CSCD被引
1
次
|
|
|
|
|
19.
Mugnier L M. Phase diversity: a technique for wave-front sensing and for diffraction-limited imaging.
Advances in Imaging and Electron Physics,2006,141:1-76
|
CSCD被引
3
次
|
|
|
|
|
20.
Labeyrie A. Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images.
Astronomy and Astrophysics,1970,6:85-87
|
CSCD被引
45
次
|
|
|
|
|
了解气象卫星更多信息，请访问