空间相机在轨成像模式的建立

李宪圣; 任建岳; 任建伟; 张星祥; 薛常喜

doi:10.3788/OPE.20152307.1852

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空间相机在轨成像模式的建立

辐射定标 | 更新时间：2020-08-12

- 空间相机在轨成像模式的建立
- Establishment of image model for on-board space camera
- 光学精密工程 2015年23卷第7期页码：1852-1858
- 作者机构：
  
  1. 长春理工大学光电工程学院,吉林长春,130022
  2. 中国科学院长春光学精密机械与物理研究所, 吉林长春 130033
- 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. 863-2-5-1-13B)()
- DOI：10.3788/OPE.20152307.1852
  中图分类号： V447.3
- 收稿日期：2015-02-15，
  
  修回日期：2015-03-10，
  
  纸质出版日期：2015-07-25
- 稿件说明：
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李宪圣, 任建岳, 任建伟等. 空间相机在轨成像模式的建立[J]. 光学精密工程, 2015,23(7): 1852-1858

LI Xian-sheng, REN Jian-yue, REN Jian-wei etc. Establishment of image model for on-board space camera[J]. Editorial Office of Optics and Precision Engineering, 2015,23(7): 1852-1858
李宪圣, 任建岳, 任建伟等. 空间相机在轨成像模式的建立[J]. 光学精密工程, 2015,23(7): 1852-1858 DOI： 10.3788/OPE.20152307.1852.

LI Xian-sheng, REN Jian-yue, REN Jian-wei etc. Establishment of image model for on-board space camera[J]. Editorial Office of Optics and Precision Engineering, 2015,23(7): 1852-1858 DOI： 10.3788/OPE.20152307.1852.

摘要

提出空间相机在轨成像模式的概念

研究了建立空间相机成像模式的方法。首先

根据太阳高角和地物反射率

使用MODTRAN软件计算相机入瞳前的辐射亮度

分析相机的辐射定标数据

包括每种成像模式的响应度、辐射亮度范围

积分时间关系等。然后

分析相机测摆成像与平飞成像时的积分时间关系

获得相机在各侧摆角下

每种成像模式的辐射亮度范围。最后

依据成像模式的辐射亮度范围和各太阳高角下景物的辐射亮度范围

建立了太阳高角和相机侧摆角组合下的成像模式表。空间相机成像时

依据成像模式表查找对应的成像模式

即可按该模式成像。该方法已多次应用于遥感相机成像实验中

获得了较好的成像效果

图像质量的满意度由65%提高到99.9%。结果表明:依据该方法建立的空间相机成像模式

获得图像效果较好

图像既包含全部景物信息又具有丰富的图像层次。

Abstract

The concept of on-board imaging model for a space camera was proposed

and the method to establish the imaging model of the space camera was researched. On the basis of the solar elevation angle and the reflection of earth surface

the radiance at the entrance pupil of space camera was calculated using the MODTRAN software. Then the radiometric calibration data were analyzed and the responsibility

radiance range and the integration time for each image model were acquired. Meanwhile

the relation between the responsibility and the integration time was obtained for scroll image and standard image and the radiance ranges at each image model was calculated at every scroll angle. Finally

according to the radiance range at each image model and the maximum objective at sensor radiance from the earth surface

an imaging model table was established under the scroll angle and solar elevation angle. When the space camera worked on board

one could choose a corresponding imaging model by looking up the table and could achieve better images. The method has been used in space camera imaging for several times

high quality remote images have been acquired. The image satisfaction improves from 65% to 99.9%. According to the method

the remote image's quality has been improved obviously. The image not only includes all scene information

but also has abundant levels.

关键词

Keywords

references

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