[1] [1] Tang Yuanhe, Chen Guangde, Zhang Chunmin, et al. O(Ⅰ,Ⅱ) forbidden lines aurora and their photochemical reactions [J]. Chinese Journal of Luminescence, 2005, 26(3): 309-315.

[2] [2] Lü Peng, Tang Yuanhe LiLu Kai, et al. Study CCD image motion for remote sensing detection [J]. Proc. of SPIE, 2007, 6279: 1-7.

[3] [3] National Oceanic and Atmospheric Administration. U. S. Standard Atmosphere[S]. 1976.

[4] [4] U. S. Standard Atmosphere 1976. MSIS and CIRA model[OL]. http://modelweb.gsfc.nasa.gov/.

[5] [5] Arun Kr Upadhayaya, Vir Singh. Correction to daytime mesospheric atomic oxygen density in MSIS-90 obtained from WINDⅡ measurements of O(1S) dayglow emissions [J]. Indian Journal of Radio & Space Physics, 2002, 31(2): 28-33.

[6] [6] Xu Jiyao, Ji Qiao, Yuan Weihua, et al. Comparison between the TIMED observed global temperature distribution and thp NRLMSISE-00 empirical atmospheric model [J]. Chin. J. Space Sci.,2006, 26(3): 177-182.

[7] [7] Sheng Peixuan, Mao Jietai, Li Jianguo, et al. Atmosphere Physics [M]. Beijing: Peking University Press, 2003.

[8] [8] Kivelson M G, Russell C T. Introduction to Space Physics [M]. Cambridge: Cambridge University Press, 1995.

[9] [9] Hedin A E. Extension of the MSIS thermospheric model into the middle and lower atmosphere [J].J. Geophys. Res., 1991, 96: 1159.

[10] [10] Picone J M, Hedin A E, Drob D P, et al.NRLMSISE-00 empirical model of the atmosphere: statistical comparisons and scientific issues [J]. J. Geophys. Res., 2002, 107(A12): 1029.

[11] [11] Chen Zhongxian. Computational Physics [M].Harbin: Harbin Institute of Technology Press,2001.