• DocumentCode
    2194800
  • Title

    The Detecting Methods of Geostationary Orbit Objects

  • Author

    Wei Min ; Chen HaiNing ; Yan TianYun ; Wu QinZhang ; Xu Bin

  • Author_Institution
    Comput. Sci. Dept., Chengdu Univ. of Inf. Technol., Chengdu, China
  • fYear
    2010
  • fDate
    2-4 April 2010
  • Firstpage
    645
  • Lastpage
    648
  • Abstract
    When optical altazimuth telescope conducting Geostationary orbit object detection, staring star and staring satellite are two ordinary work mode. This article proposes two different kinds of object detection methods based on the characteristic of object imaging of above two work mode. When staring star, symmetrical difference is presented to reduce star interference, and remaining star interference can be further reduced by correlating the object characteristic of the adjacent two frames. And staring satellite, a modified difference is presented. The adjacent two frames are differented twice, star interference is reduced, target objects are binary and marked, and objects are detected by the logical most neighboring method finally. Results of experiment indicates Geostationary orbit objects can be detected precisely and effectively by using this two detection methods.
  • Keywords
    astronomical image processing; astronomical telescopes; geology; object detection; stars; geostationary orbit objects detecting methods; object detection methods; optical altazimuth telescope; star interference; Earth; Humans; Information technology; Interference; Object detection; Optical imaging; Rockets; Satellite broadcasting; Space technology; Telescopes; Binary statistical filte; Geostationary orbit; Optical telescope; Symmetrical difference; logical most neighboring method;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Intelligent Information Technology and Security Informatics (IITSI), 2010 Third International Symposium on
  • Conference_Location
    Jinggangshan
  • Print_ISBN
    978-1-4244-6730-3
  • Electronic_ISBN
    978-1-4244-6743-3
  • Type

    conf

  • DOI
    10.1109/IITSI.2010.31
  • Filename
    5453706