• Opto-Electronic Engineering
  • Vol. 40, Issue 6, 6 (2013)
HU Miao*, XU Guorui, ZHANG Hui, HUANG Qianfeng, ZHANG Fei, DENG Jing, and LIU Chenxi
Author Affiliations
  • [in Chinese]
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    DOI: 10.3969/j.issn.1003-501x.2013.06.002 Cite this Article
    HU Miao, XU Guorui, ZHANG Hui, HUANG Qianfeng, ZHANG Fei, DENG Jing, LIU Chenxi. Star Magnitude Measurement of Geosynchronous Orbit Cube Target[J]. Opto-Electronic Engineering, 2013, 40(6): 6 Copy Citation Text show less

    Abstract

    According to the definition of satellite’s magnitude, for geosynchronous orbit space satellite, the theoretical computing model of star magnitude was built. Space vectors among sun, observation station and target satellite were derived to calculate the time-space relationship parameters. The simulation curves of magnitude vs. time were drawn based on the model and corresponding parameters. The simulation results were verified to match the experiments ones by using satellite targeting system and astronomical telescope. At last, one geosynchronous satellite with 13.4 magnitudes was observed.
    HU Miao, XU Guorui, ZHANG Hui, HUANG Qianfeng, ZHANG Fei, DENG Jing, LIU Chenxi. Star Magnitude Measurement of Geosynchronous Orbit Cube Target[J]. Opto-Electronic Engineering, 2013, 40(6): 6
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