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Research on the autonomous star sensor based on indirectly sensing horizon and its optical design
Wu, Y.; X. Zhang; J. Zhang; L. Wang; H. Qu; Y. Zhu and F. Zeng
2015
发表期刊Guangxue Xuebao/Acta Optica Sinica
卷号35期号:2
摘要Based on stellar refraction indirectly sensing of autonomous navigation for horizon star sensor, a parameter design is analyzed for stellar refraction star sensor which is included by detect waveband, observation field, detect probability and threshold value of magnitude. The field of view (FOV) of star sensor is divided into two parts of refraction star and unrefraction star. The FOV decreases as orbit attitude increases. Limited by atmosphere absorption, the waveband needs to be 600~900 nm, and the signal-to-noise ratio (SNR) decreases as atmosphere height increases. High sensitive back-thinned charge coupled device (CCD) is applied and athermalizing optical system design is achieved. The result shows that imaging quality is good enough and measure precision of single star sensor achieves 1, which can meet the requirement of autonomous star sensor measure precision. , 2015, Chinese Optical Society. All right reserved.
文章类型期刊论文
收录类别EI
文献类型期刊论文
条目标识符http://ir.ciomp.ac.cn/handle/181722/56201
专题中科院长春光机所知识产出
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GB/T 7714
Wu, Y.,X. Zhang,J. Zhang,et al. Research on the autonomous star sensor based on indirectly sensing horizon and its optical design[J]. Guangxue Xuebao/Acta Optica Sinica,2015,35(2).
APA Wu, Y.,X. Zhang,J. Zhang,L. Wang,H. Qu,&Y. Zhu and F. Zeng.(2015).Research on the autonomous star sensor based on indirectly sensing horizon and its optical design.Guangxue Xuebao/Acta Optica Sinica,35(2).
MLA Wu, Y.,et al."Research on the autonomous star sensor based on indirectly sensing horizon and its optical design".Guangxue Xuebao/Acta Optica Sinica 35.2(2015).
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