[1]刘瑞斌. 天文用光纤特性的研究[D]. 长春:长春理工大学,2002. LIU Rui-bin. The study on fibers in astronomy[D]. Changchun: Changchun University of Science and Technology, 2002. (in Chinese) [2]HU Hong-zhuan, XING Xiao-zheng, ZHAI Chao, et al. New type optical fiber positioning unit device for LAMOST[C]. Waikoloa, HI, USA: Large Groundbased Telescopes (SPIE) Conference, 2003. [3]HUNTER T R, RAMSEY L W. Scrambling properties of optical fibers and the performance of a double scrambler[J]. Astronomical Society of the Pacific, 1992, 104(682): 1244-1251. [4]郑史烈,章献民,陈抗生. 塑料光纤的远场辐射图和微分模式损耗研究[J]. 光子学报,2003, 32(12): 1334-1337. ZHENG Shi-lie, ZHANG Xian-min, CHEN Kang-sheng. Far field pattern and differential mode attenuation of POF[J]. Acta Photonica Sinica, 2003, 32(12): 1334-1337. (in Chinese with an English abstract) [5]AVILA G, SINGH P, ALBERTSEN M. Photometrical scrambling gain and focal ratio degradation in fibers for astronomical instruments[C]. Orlando, FL, USA: Groundbased and Airborne Instrumentation for Astronomy (SPIE) Conference, 2006. [6]AVILA G, BUZZONI B. Fiber characterization and compact scrambler at ESO[C]. Kona, HI, USA: Optical Astronomical Instrumentation (SPIE) Conference, 1998. [7]AVILA G, SINGH P, ALBERTSEN M. A high-efficiency fibre double-scrambler prototype[C]. San Diego, California, USA: Ground-based and Airborne Instrumentation for Astronomy III (SPIE) Conference, 2010. [8]AVILA G, KOHLER D, ARAYA M, et al. Performances of HARPS and FEROS fibres in La Silla ESO Observatory[C]. Glasgow, Scotland, United Kingdom: Ground-based Instrumentation for Astronomy (SPIE) Conference, 2004. [9]AVILA G, SINGH P. Optical fiber scrambling and light pipes for high accuracy radial velocities measurements[C]. Marseille, France: Advanced Optical and Mechanical Technologies in Telescopes and Instrumentation (SPIE) Conference, 2008. [10]吴重庆. 光波导理论[M]. 第2版. 北京:清华大学出版社,2005. WU Chong-qing. Optical waveguide theory[M]. 2nd Edition. Beijing: Tsinghua University Press, 2005. (in Chinese)
|