中波红外整层大气透过率测量及误差分析

刘俊池; 李洪文; 王建立; 殷丽梅; 李宏壮; 张振铎

doi:10.3788/OPE.20152306.1547

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中波红外整层大气透过率测量及误差分析

现代应用光学 | 更新时间：2020-08-13

- 中波红外整层大气透过率测量及误差分析
- Measurement of mid-infrared total atmospheric transmittance and its error analysis
- 光学精密工程 2015年23卷第6期页码：1547-1557
- 作者机构：
  
  1. 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
  2. 中国科学院大学北京,中国,100049
- 作者简介：
- 基金信息：
  
  国家863高技术研究发展计划资助项目(No.2013AAXXX1009)()
- DOI：10.3788/OPE.20152306.1547
  中图分类号： P407.5;TP732+.2
- 收稿日期：2014-06-25，
  
  修回日期：2014-08-19，
  
  纸质出版日期：2015-06-25
- 稿件说明：
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刘俊池, 李洪文, 王建立等. 中波红外整层大气透过率测量及误差分析[J]. 光学精密工程, 2015,23(6): 1547-1557

LIU Jun-chi, LI Hong-wen, WANG Jian-li etc. Measurement of mid-infrared total atmospheric transmittance and its error analysis[J]. Editorial Office of Optics and Precision Engineering, 2015,23(6): 1547-1557
刘俊池, 李洪文, 王建立等. 中波红外整层大气透过率测量及误差分析[J]. 光学精密工程, 2015,23(6): 1547-1557 DOI： 10.3788/OPE.20152306.1547.

LIU Jun-chi, LI Hong-wen, WANG Jian-li etc. Measurement of mid-infrared total atmospheric transmittance and its error analysis[J]. Editorial Office of Optics and Precision Engineering, 2015,23(6): 1547-1557 DOI： 10.3788/OPE.20152306.1547.

摘要

为实现中波红外整层大气透过率的现场测量

提高空间目标红外辐射特性测量精度

研究了基于标准红外自然星的大气透过率测量方法.建立了基于Beer定律和Langley-Plot定标原理的测量实验数学模型

搭建了基于1.2 m口径地基光电望远镜的测量实验系统.采用了准实时单点校正窗口提取和信噪比特性曲线等方法有效降低了红外探测器非均匀性和自然星弥散成像等问题给测量精度带来的影响.最后

分析了测量实验的理论误差.实验数据显示:空间目标大气层外红外辐射照度测量的最大实际误差为16.28%

中波红外整层大气透过率测量的理论误差为11.75%.结果表明:基于标准红外自然星的大气透过率测量方法测量误差小

实验系统对外场观测任务适应性强

为空间目标红外辐射特性的地基测量提供了新的解决方案.

Abstract

To measure the mid-infrared total atmospheric transmittance in a field and to improve the measuring accuracy of infrared radiation of spatial objects

a measuring method based on standard infrared stars was discussed. A mathematical model based on Beer's law and Langley-Plot calibration principle was established

and an experimental system based on the ground-based optic-electric telescope with an aperture of 1.2 m was set up. Then

Quasi-real-time One-point Correction Method

Window-extracted Method and SNR Characteristic Curve were employed to reduce the effects of the non-uniformity of detectors and the diffusion imaging of stars on the measuring accuracy. Finally

the error of the measurement in the experiments was analyzed.Experiments and analysis show that the maximum measuring error of the infrared radiation illumination of spatial objects is 16.28%

and the theoretical measuring error of mid-infrared total atmospheric transmittance is 11.75%.The results indicate that the measuring method proposed in this pape has a smaller measuring error

the experimental system is adapt to observation missions in the field and it provides a new solution for measuring the infrared radiation of spatial objects.

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references

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