全天时星敏感器的建模分析与实验验证

王文杰; 张广军; 魏新国

doi:10.3788/IRLA201948.1113001

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全天时星敏感器的建模分析与实验验证

王文杰, 张广军, 魏新国

文章导航 > 红外与激光工程 > 2019 > 48(11): 1113001-1113001(7)

王文杰, 张广军, 魏新国. 全天时星敏感器的建模分析与实验验证[J]. 红外与激光工程, 2019, 48(11): 1113001-1113001(7). doi: 10.3788/IRLA201948.1113001

引用本文:

王文杰, 张广军, 魏新国. 全天时星敏感器的建模分析与实验验证[J]. 红外与激光工程, 2019, 48(11): 1113001-1113001(7). doi: 10.3788/IRLA201948.1113001

Wang Wenjie, Zhang Guangjun, Wei Xinguo. Modeling analysis and experimental verification for all-time star sensor[J]. Infrared and Laser Engineering, 2019, 48(11): 1113001-1113001(7). doi: 10.3788/IRLA201948.1113001

Citation:

Wang Wenjie, Zhang Guangjun, Wei Xinguo. Modeling analysis and experimental verification for all-time star sensor[J]. Infrared and Laser Engineering, 2019, 48(11): 1113001-1113001(7). doi: 10.3788/IRLA201948.1113001

全天时星敏感器的建模分析与实验验证

doi: 10.3788/IRLA201948.1113001

1.
北京航空航天大学仪器科学与光电工程学院精密光机电一体化技术教育部重点实验室,北京 100191

基金项目:

国家自然科学基金（61378052）;国家自然科学青年科学基金（61705005，61605007）

详细信息

作者简介:
王文杰(1988-),男,博士生,主要从事天体敏感器方面的研究。Email:wangwenjiejing@126.com

中图分类号: V448.2

Modeling analysis and experimental verification for all-time star sensor

1.
Key Laboratory of Precision Opto-mechatronics Technology,Ministry of Education,School of Instrumental Science and Opto-electronics Engineering,Beihang University,Beijing 100191,China

摘要: 全天时星敏感器技术可以将星敏感器的应用推广到临近空间飞行器如平流层飞艇和高空气球等平台，是星敏感器未来发展的一个重要方向。由于白天受到强烈的大气背景辐射的影响，可见光波段星敏感器的探测能力显著受限。大气背景辐射在短波红外处的强度迅速降低，因此利用短波红外成像系统在0.9~1.7m波段下进行恒星探测成为研究全天时星敏感器技术的一种有效可行的方案。为了系统地分析并验证短波红外全天时星敏感器的可行性，文中在分析全天时星敏感器探测模型的基础上，重点讨论了短波红外探测器噪声对星敏感器探测能力的影响并基于探测模型确定了20 km高度处全天时星敏感器的光学参数。基于短波红外探测器研制了全天时星敏感器原理样机，结合地面处的观星实验，测试了原理样机的探测性能并验证了全天时星敏感器探测模型的正确性。
- 全天时星敏感器 /
- 建模仿真 /
- 短波红外探测器噪声 /
- 外场白天观星实验
Abstract: As an important direction for the future development of star sensors, all-time star sensor technology can extend the application of star sensors to near space platforms such as stratospheric airships and high-altitude balloons. Due to the intense atmospheric background radiation during daytime, the detection capability of star sensors in visible band was significantly limited. The intensity of atmospheric background radiation in the short-wave infrared (SWIR) band was rapidly reduced compared to that in the visible detection band. Therefore, the application of SWIR imaging systems for star detection in the range of 0.9-1.7 m has become an effective solution for studying the all-time star sensor technology. In order to analyze and verify the feasibility of SWIR all-time star sensor, the all-time star sensor detection model was analyzed and the impact of SWIR detector noise on the detection capability was discussed in this paper. Then, the optical parameters of the all-time star sensor at a height of 20 km were determined through simulation calculation. The prototype of the all-time star sensor was developed based on SWIR detector. Combined with the star observation experiments at the ground, the detection performance of the prototype was tested and the correctness of the all-time sensor detection model was verified.
- all-time star sensor /
- modeling and simulation /
- short-wave infrared detector noise /
- daytime star observation experiments

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全天时星敏感器的建模分析与实验验证

doi: 10.3788/IRLA201948.1113001

1. 北京航空航天大学仪器科学与光电工程学院精密光机电一体化技术教育部重点实验室,北京 100191

作者简介:
王文杰(1988-),男,博士生,主要从事天体敏感器方面的研究。Email:wangwenjiejing@126.com

收稿日期: 2019-07-05
修回日期: 2019-08-15
刊出日期: 2019-11-25

基金项目:

国家自然科学基金（61378052）;国家自然科学青年科学基金（61705005，61605007）

中图分类号: V448.2

关键词:

摘要: 全天时星敏感器技术可以将星敏感器的应用推广到临近空间飞行器如平流层飞艇和高空气球等平台，是星敏感器未来发展的一个重要方向。由于白天受到强烈的大气背景辐射的影响，可见光波段星敏感器的探测能力显著受限。大气背景辐射在短波红外处的强度迅速降低，因此利用短波红外成像系统在0.9~1.7m波段下进行恒星探测成为研究全天时星敏感器技术的一种有效可行的方案。为了系统地分析并验证短波红外全天时星敏感器的可行性，文中在分析全天时星敏感器探测模型的基础上，重点讨论了短波红外探测器噪声对星敏感器探测能力的影响并基于探测模型确定了20 km高度处全天时星敏感器的光学参数。基于短波红外探测器研制了全天时星敏感器原理样机，结合地面处的观星实验，测试了原理样机的探测性能并验证了全天时星敏感器探测模型的正确性。

English Abstract

Modeling analysis and experimental verification for all-time star sensor

1. Key Laboratory of Precision Opto-mechatronics Technology,Ministry of Education,School of Instrumental Science and Opto-electronics Engineering,Beihang University,Beijing 100191,China

Received Date: 2019-07-05
Rev Recd Date: 2019-08-15
Publish Date: 2019-11-25

Keywords:

Abstract: As an important direction for the future development of star sensors, all-time star sensor technology can extend the application of star sensors to near space platforms such as stratospheric airships and high-altitude balloons. Due to the intense atmospheric background radiation during daytime, the detection capability of star sensors in visible band was significantly limited. The intensity of atmospheric background radiation in the short-wave infrared (SWIR) band was rapidly reduced compared to that in the visible detection band. Therefore, the application of SWIR imaging systems for star detection in the range of 0.9-1.7 m has become an effective solution for studying the all-time star sensor technology. In order to analyze and verify the feasibility of SWIR all-time star sensor, the all-time star sensor detection model was analyzed and the impact of SWIR detector noise on the detection capability was discussed in this paper. Then, the optical parameters of the all-time star sensor at a height of 20 km were determined through simulation calculation. The prototype of the all-time star sensor was developed based on SWIR detector. Combined with the star observation experiments at the ground, the detection performance of the prototype was tested and the correctness of the all-time sensor detection model was verified.