DocumentCode
2105143
Title
Research on Temperature Field for Spacial Solar Array
Author
Sun Chuang ; Xia Xinlin ; Li Defu ; Li Yi
Author_Institution
Sch. of Energy Sci. & Eng., Harbin Inst. of Technol., Harbin, China
fYear
2010
fDate
28-31 March 2010
Firstpage
1
Lastpage
4
Abstract
The solar array which provides most of energy for the satellite plays a very important role. And the conversion coefficient of solar cell used in the solar array is directly influenced by the array temperature, which is also responsibility for the stability and safety of satellite, especially for the solar array. This paper discusses the solar array temperature fields under different situations, including the periods of the satellite operating in spring, summer and winter. Obtaining the incidence angle of the solar array in the three periods, the radiative heat flux is computed by Monte Carlo method (MCM) and the finite volume method (FVM) is employed to win the temperature field, with the harmonic mean value being used for the heat transfer at interface between different materials. The results show that, the temperature fields of the solar array are quite different for various seasons, and the highest temperature of the array is 308 K in spring, the lowest temperature is 225 K in summer, which is caused by the shadow of the earth.
Keywords
Monte Carlo methods; finite volume methods; solar cell arrays; Monte Carlo method; finite volume method; harmonic mean value; heat transfer; radiative heat flux; solar array temperature fields; solar cells; spacial solar array; Computer interfaces; Finite volume methods; Heat transfer; Photovoltaic cells; Radiation safety; Satellites; Solar heating; Springs; Stability; Temperature;
fLanguage
English
Publisher
ieee
Conference_Titel
Power and Energy Engineering Conference (APPEEC), 2010 Asia-Pacific
Conference_Location
Chengdu
Print_ISBN
978-1-4244-4812-8
Electronic_ISBN
978-1-4244-4813-5
Type
conf
DOI
10.1109/APPEEC.2010.5448902
Filename
5448902
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