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11 September 2013 The calculation model of the satellite solar panels infrared feature
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Proceedings Volume 8907, International Symposium on Photoelectronic Detection and Imaging 2013: Infrared Imaging and Applications; 89075K (2013) https://doi.org/10.1117/12.2035035
Event: ISPDI 2013 - Fifth International Symposium on Photoelectronic Detection and Imaging, 2013, Beijing, China
Abstract
The infrared radiation change of the solar panels is an obvious feature to tell whether they are working normally or not. In this paper, the calculation model of the satellite's solar panels infrared feature is established. First, combined with the parameter descriptions of the satellite's six orbital elements and with the use of the coordinate transformation method, the calculation formulas of the radiation flux that the solar panels get from the sun and the earth are derived, no matter which location of the satellite in orbit. Second, the calculation model of the solar panels' temperature field is established, and the equations are solved numerically with the boundary condition of radiation heat flux. Finally, the calculation models of the solar panels' infrared radiation in 3~5μm band and 8~14μm band are established, and the equations are solved numerically, thinking differently about their radiation and reflected radiation.
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Li Yang, Xiang-yin Lv, Wei Jin, Hua Yang, and Ji-jin Zhao "The calculation model of the satellite solar panels infrared feature", Proc. SPIE 8907, International Symposium on Photoelectronic Detection and Imaging 2013: Infrared Imaging and Applications, 89075K (11 September 2013); https://doi.org/10.1117/12.2035035
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