应用科学学报 ›› 2017, Vol. 35 ›› Issue (1): 90-98.doi: 10.3969/j.issn.0255-8297.2017.01.010

• 信号与信息处理 • 上一篇    下一篇

微小卫星低照度遥感成像的信噪比

张洋1,2, 钟兴1,3   

  1. 1. 中国科学院 长春光学精密机械与物理研究所, 长春 130033;
    2. 中国科学院大学, 北京 100039;
    3. 长光卫星技术有限公司, 长春 130102
  • 收稿日期:2016-04-29 修回日期:2016-08-11 出版日期:2017-01-30 发布日期:2017-01-30
  • 作者简介:钟兴,研究员,博导,研究方向:星载一体化,E-mail:ciomper@163.com

Signal-to-Noise Ratio in Low Light Images from Microsatellite

ZHANG Yang1,2, ZHONG Xing1,3   

  1. 1. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Science, Changchun 130033, China;
    2. University of Chinese Academy of Sciences, Beijing 100039, China;
    3. Chang Guang Satellite Technology Co., Ltd., Changchun 130102, China
  • Received:2016-04-29 Revised:2016-08-11 Online:2017-01-30 Published:2017-01-30

摘要:

为了实现低照度环境下遥感图像的正常采集,对遥感平台与遥感传感器进行了研究.分析对比了微小卫星平台现有遥感图像成像模式,利用敏捷性微小卫星平台,提出了在凝视模式下增加积分时间获取星载卫星低照度图像的方法,并对凝视情况下遥感图像信噪比进行建模和分析,给出了遥感图像信噪比与光学系统相对孔径、积分时间之间的函数关系.搭建了实验平台,可实现在低照度环境下进行不同积分时间的实际靶标图像采集及信噪比分析.

关键词: 低照度成像, 积分时间, 卫星姿态, 遥感成像, 凝视模式, 信噪比

Abstract:

To acquire low-light remote sensing images, remote sensing platform and sensors are studied.By increasing integration time, low-light remote images are combined.In contrast to the current imaging models we have on satellite, a staring imaging model can achieve longer integer time.The new microsatellite platform can collect low-light remote image in this model.A mathematical model for signal-to-noise ratio is established to obtain functional relationship among relative optical aperture, integration time and signal-to-noise ratio.An experimental platform is setup to collect target images acquired in a low light environment with different integration time for analysis of signal-to-noise ratio.

Key words: low-light image, satellite posture, signal-to-noise ratio, remote sensing image, integration time, staring imaging model

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