空间相机焦平面CCD交错拼接重叠像元数计算

武奕楠; 李国宁; 张宇

doi:10.3788/OPE.20162402.0422

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空间相机焦平面CCD交错拼接重叠像元数计算

信息科学 | 更新时间：2020-08-13

- 空间相机焦平面CCD交错拼接重叠像元数计算
- Calculation of overlapping pixels in interleaving assembly for CCD focal plane of space camera
- 光学精密工程 2016年24卷第2期页码：422-429
- 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：
  
  吉林省科技发展计划资助项目(No.20130522107JH)()
- DOI：10.3788/OPE.20162402.0422
  中图分类号： V447.3;TN386.5
- 收稿日期：2015-04-17，
  
  修回日期：2015-06-25，
  
  纸质出版日期：2016-02-25
- 稿件说明：
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武奕楠, 李国宁, 张宇. 空间相机焦平面CCD交错拼接重叠像元数计算[J]. 光学精密工程, 2016,24(2): 422-429

WU Yi-nan, LI Guo-ning, ZHANG Yu. Calculation of overlapping pixels in interleaving assembly for CCD focal plane of space camera[J]. Editorial Office of Optics and Precision Engineering, 2016,24(2): 422-429
武奕楠, 李国宁, 张宇. 空间相机焦平面CCD交错拼接重叠像元数计算[J]. 光学精密工程, 2016,24(2): 422-429 DOI： 10.3788/OPE.20162402.0422.

WU Yi-nan, LI Guo-ning, ZHANG Yu. Calculation of overlapping pixels in interleaving assembly for CCD focal plane of space camera[J]. Editorial Office of Optics and Precision Engineering, 2016,24(2): 422-429 DOI： 10.3788/OPE.20162402.0422.

摘要

针对大视场空间相机焦平面采用的多片CCD交错拼接

提出了一种适用于多种姿态模式的重叠像元数解析计算方法

以保证空间相机成像视场中不出现漏缝。分析了CCD交错拼接的成像特性和产生漏缝的原因;基于空间坐标系变换和中心投影共线方程建立了重叠像元数计算模型

对像点、相机摄像中心、地面景物点建立动态数学关系

通过追踪像点在像面上的运动轨迹计算了拼接缝像元重叠情况。结合实际工程样例

计算和分析了空间相机机动角度、星下点纬度、视场位置等因素对重叠像元数的影响

并将各工况下计算的最多漏像元数作为最终拼接量。结果表明:重叠像元数理论误差小于1 pixel;对比侧摆

俯仰成像时所需拼接像元数更多;该计算模型可扩展应用于其他类型空间相机在任何姿态模式下的重叠像元数计算。

Abstract

The focal plane of a wide-field space camera is comprised of several staggered Charge Coupled Device(CCD) detectors.To eliminate the gap in imaging field of the space camera

this paper proposes an analytic calculation method for overlapping pixels applied to multiple maneuvering angle modes. The imaging characteristics of CCD interleaving assembly and the reason that imaging gaps appear were analyzed. Then

the calculation model for overlapping pixels was established by combining space coordinate transformation with a collinearity equation. The dynamic mathematical relationship of the image point

camera center and the ground point was established. The overlapping pixels between adjacent CCDs were calculated by tracing the locus of image point on the image plane. With an engineering example

the influence of maneuvering angle

subastral latitude and the field location of the space camera on overlapping pixels was calculated and analyzed and the maxmum number of gap pixels calculating among different working situations were considered as mechanical assembly numbers. The result shows that the theoretical error of the number overlapping pixels is less than 1 pixel. Comparing with scrolling imaging

the pitching imaging needs more number of assembly pixels. The computing model can be applied to other space cameras of different types

and the overlapping pixels can be calculated at any attitude mode.

关键词

Keywords

references

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