光学学报, 2007, 27 (8): 1490, 网络出版: 2007-09-05   

改型萨尼亚克成像干涉仪的光通量

Optical Throughput of Modified Sagnac Imaging Interferometer
作者单位
1 西安理工大学理学院, 西安 710048
2 西安交通大学理学院, 西安 710049
摘要
根据菲涅耳公式,通过计算超广角萨尼亚克干涉仪各面的反射、透射系数,得出干涉仪的透射率、出射立体角,最后推导出光通量的具体表达式。代入改型萨尼亚克干涉仪两臂玻璃ZBaF17和QF14尺寸和折射率等参量,得出超广角萨尼亚克干涉仪的出射光强是入射光强的0.4397倍,立体角为1.7316×10-4 sr,AΩ=0.4×10-4 cm2·sr。
Abstract
According to Fresnell's formula, the coefficients of reflection and transmission of every interface of super-wide-angle Sagnac interferometer (SASI) are calculated. The exit solid angle and transmissivity are deduced, and the expression of luminous flux is derived. The luminous flux optical throughput is calculated with the parameters such as sizes and reflective index of glass arms of ZBaF17 and QF14 in a modified super-wide-angle Sagnac interferometer. The solid angle is 1.7316×10-4 rad, the emergent intensity is about 0.4397 of incidence, with AΩ=0.4×10-4 cm2·sr.
参考文献

[1] G. G. Shepherd, G. Thullier, W. A. Gault et al.. WINDⅡ, the wind imaging interferometer on the upper atmosphere research satellite[J]. J. Geophysical Research, 1993, 98(D6): 10725~10750

[2] I. C. McDade,G. G. Shepherd,W. A. Gault et al.. The stratospheric wind interferometer for transport studies (SWIFT)[C]. IEEE, 2001, 3: 1344~1346

[3] William Gault,Stoyan Sargoytchev,Stephen Brown. Divided mirror technique for measuring Doppler shifts with a Michelson interferometer[C]. Proc. SPIE, 2001, 4306: 266~272

[4] Leonard John Otten Ⅳ, Andrew D. Meigs,Frederick P. Porrigal et al.. MightySat Ⅱ. 1: An optical design and performance update[C]. Proc. SPIE, 1997, 2957: 390~398

[5] Gao Zhan, Xiang Libin, An Baoqing et al.. A novel imaging in interferometry[J]. J. Optoelectronics·Laser, 1998, 9(2): 116~118 (in Chinese)
高瞻,相里斌,安葆青 等. 一种新型成像干涉光谱技术[J]. 光电子·激光, 1998, 9(2): 116~118

[6] . . Measurement atmospheric wind field with wide-angle modified Sagnac interferometer by satellite′s pushbroom mode[J]. Progress in Nature Science, 2006, 16(11): 1491-1495.

[7] Yuanhe Tang, Guangde Chen, Chunmin Zhang et al.. Optimization of the modified Sagnac imaging interferometer for full compensation[C]. Proc. SPIE, 2007, 6279: 62791G-1-6

[8] Tang Yuanhe. Study of the Wind Measurement of the Upper Atmosphere by the Imaging Interferometry Technology[D]. Xi′an: Xi′an Jiaotong University,2006. 42~73 (in Chinese)
唐远河. 成像干涉技术探测上层大气风场的研究[D]. 西安: 西安交通大学, 2006. 42~73

[9] Zhang Chunmin, Zhao Baochang, Xiang Libin et al.. Analysis and calculation of throughput of the polarization interference imaging spectrometer[J]. Acta Optica Sinica, 2001, 21(2): 192~197 (in Chinese)
张淳民,赵葆常,相里斌 等. 偏振干涉成像光谱仪通量的分析与计算[J]. 光学学报, 2001, 21(2): 192~197

[10] Michael R. Descour. The throughput advantage in imaging Fourier-transform spectrometers[C]. Proc. SPIE, 1996, 2819: 285~290

[11] . L. Junttila,J. Kauppinen, E. Ikonen. Performance limits of stationery Fourier spectrometers[J]. J. Opt. Soc. Am. A, 1991, 8(9): 1457-1462.

[12] Tang Yuanhe, Zhang Chunmin, He Jian et al.. Study of the detection mode of upper atmospheric wind field based on Lorentzian profile aurora[J]. Acta Optica Sinica, 2005, 25(6): 721~725 (in Chinese)
唐远河,张淳民,贺健 等. 基于洛伦兹线型极光的上层大气风场探测模式研究[J]. 光学学报, 2005, 25(6): 721~725

[13] . G. Shepherd,W. A. Gault,D. W. Miller et al.. WAMDⅡ: wide-angle Michelson Doppler imaging interferometer for spacelab[J]. Appl. Opt., 1985, 24(11): 1571-1584.

唐远河, 陈光德, 赵振宇, 张淳民. 改型萨尼亚克成像干涉仪的光通量[J]. 光学学报, 2007, 27(8): 1490. 唐远河, 陈光德, 赵振宇, 张淳民. Optical Throughput of Modified Sagnac Imaging Interferometer[J]. Acta Optica Sinica, 2007, 27(8): 1490.

本文已被 2 篇论文引用
被引统计数据来源于中国光学期刊网
引用该论文: TXT   |   EndNote

相关论文

加载中...

关于本站 Cookie 的使用提示

中国光学期刊网使用基于 cookie 的技术来更好地为您提供各项服务,点击此处了解我们的隐私策略。 如您需继续使用本网站,请您授权我们使用本地 cookie 来保存部分信息。
全站搜索
您最值得信赖的光电行业旗舰网络服务平台!