小视场绝对辐射计视场测量及修正项计算

杨振岭; 方伟; 王凯; 姜明; 宋宝奇

doi:10.3788/OPE.20132104.0870

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小视场绝对辐射计视场测量及修正项计算

现代应用光学 | 更新时间：2020-08-12

- 小视场绝对辐射计视场测量及修正项计算
- Field of View Measurement and Correction Term Calculation for Small-Field Radiometer
- 光学精密工程 2013年21卷第4期页码：870-875
- 作者机构：
  
  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
- 作者简介：
- 基金信息：
  
  航天光谱仪新理念高精度在轨绝对辐射定标方法研究()
- DOI：10.3788/OPE.20132104.0870
  中图分类号： V443.5;TP73
- 收稿日期：2012-11-12，
  
  修回日期：2013-01-22，
  
  网络出版日期：2013-04-20，
  
  纸质出版日期：2013-04-15
- 稿件说明：
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杨振岭方伟王凯姜明宋宝奇. 小视场绝对辐射计视场测量及修正项计算[J]. 光学精密工程, 2013,21(4): 870-875

YANG Zhen-Ling FANG Wei WANG Kai JIANG Ming SONG Bao-qi. Field of View Measurement and Correction Term Calculation for Small-Field Radiometer[J]. Editorial Office of Optics and Precision Engineering, 2013,21(4): 870-875
杨振岭方伟王凯姜明宋宝奇. 小视场绝对辐射计视场测量及修正项计算[J]. 光学精密工程, 2013,21(4): 870-875 DOI： 10.3788/OPE.20132104.0870.

YANG Zhen-Ling FANG Wei WANG Kai JIANG Ming SONG Bao-qi. Field of View Measurement and Correction Term Calculation for Small-Field Radiometer[J]. Editorial Office of Optics and Precision Engineering, 2013,21(4): 870-875 DOI： 10.3788/OPE.20132104.0870.

摘要

风云三号A星和B星上搭载的太阳辐射监测仪由于视场较大而引入较多不确定因素，因此风云三号C星太阳辐射监测仪采用小视场绝对辐射计来跟踪太阳测量。本文研究了小视场绝对辐射计视场带来的修正因素。计算了C星太阳辐射监测仪由视场光栏和主光栏确定的视场大小；基于此视场计算值，给出了仪器辐照度测量值随光源入射角变化的理论曲线；并且利用实验室搭建的视场测量装置，对此变化曲线进行了实际测量。结果表明，测量曲线与理论曲线的相对偏差平均为1%～2%，接近测量装置的极限精度，从而验证了视场计算值的准确性。利用计算视场评价了在轨测量时辐射计与冷空间背景的辐射交换修正项，结果显示，小视场会对太阳辐射测量产生2.023 W/m

的冷空间背景修正，相对太阳辐照度测量精度要求

修正项计算标准差可以忽略。

Abstract

Solar Irradiance Monitor (SIM) on the FY-3C satellite was designed to be a Small-field-of-view Radiometer (SFoV-R) with a precise solar pointing system to decrease the measurement uncertainty derived from the wide field-of-view of SIM on FY-3A and FY-3B satellites. To obtain the measurement uncertainty derived from the SFoV-R

the field-of-view of SFoV-R on FY-3C satellite determined by a view-limiting aperture and a precision aperture was calculated. Based on this field-of-view

a theoretical change curve of the measured irradiance incidence angle was achieved. Then

an actual measurement of the change curves was performed. The result indicates that the relative deviation on an average between the theoretical and measured change curves is 1%-2%

which is close to the limit accuracy of the measuring installation and proves the veracity of the calculated values for field-of-view. The correction term of radiation exchange between space and the radiometer is estimated to be 2.023 W/m2 based on the calculated field-of-view. Experiments show that the standard deviation of this correction term can be neglected compared to the requirement of solar irradiance measurement accuracy.

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references

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