小型宽光谱太阳光谱仪光学设计

高震宇; 方伟; 张浩; 杨振岭; 王玉鹏

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小型宽光谱太阳光谱仪光学设计

高震宇, 方伟, 张浩, 杨振岭, 王玉鹏

文章导航 > 红外与激光工程 > 2015 > 44(2): 590-595

高震宇, 方伟, 张浩, 杨振岭, 王玉鹏. 小型宽光谱太阳光谱仪光学设计[J]. 红外与激光工程, 2015, 44(2): 590-595.

引用本文:

高震宇, 方伟, 张浩, 杨振岭, 王玉鹏. 小型宽光谱太阳光谱仪光学设计[J]. 红外与激光工程, 2015, 44(2): 590-595.

Gao Zhenyu, Fang Wei, Zhang Hao, Yang Zhenling, Wang Yupeng. Design of a small-size solar spectrograph with wide spectral range[J]. Infrared and Laser Engineering, 2015, 44(2): 590-595.

Citation:

Gao Zhenyu, Fang Wei, Zhang Hao, Yang Zhenling, Wang Yupeng. Design of a small-size solar spectrograph with wide spectral range[J]. Infrared and Laser Engineering, 2015, 44(2): 590-595.

小型宽光谱太阳光谱仪光学设计

高震宇^1,2,
方伟¹,
张浩^1,2,
杨振岭¹,
王玉鹏¹

1.
中国科学院长春光学精密机械与物理研究所,吉林长春130033;
2.
中国科学院大学,北京100049

基金项目:

国家自然科学基金(41227003)

详细信息

作者简介:
高震宇(1988-),男,博士生,主要从事空间光谱仪器光学设计方面的研究。Email:lnsygzy92@zju.edu.cn

中图分类号: O433;TH744

Design of a small-size solar spectrograph with wide spectral range

1.
Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences,Changchun 130033,China;
2.
University of Chinese Academy of Sciences,Beijing 100049,China

摘要: 针对大气层外的太阳光谱辐照度监测,设计了一种星载小型宽光谱太阳光谱仪。光学系统应用改进的切尔尼-特纳光学结构,工作波长范围为600~1 200 nm(二级光谱)和1 200~2 400 nm(一级光谱);一二级光谱使用二向色分光镜分离,并采用两片线阵探测器同时接收,实现全谱瞬态直读。整个光学结构的尺寸为80 mm55 mm20 mm。经过系统优化,全谱段子午方向像差低于6 m。基于惠更斯点扩散函数(PSF),仿真探测器像元的光谱响应函数(SRF),结果表明光谱分辨率在600~1 200 nm波段优于2 nm,在1 200~2 400 nm波段优于4 nm。系统结构简单紧凑,稳定性高,适合用于空间太阳光谱辐照度的在轨监测。
- 太阳光谱仪 /
- 二向色分光镜 /
- 点扩散函数 /
- 光谱响应函数
Abstract: A small-size satellite-borne solar spectrograph with wide spectral range was designed to monitor the Solar Spectral Irradiance (SSI) outside the atmosphere. The instrument used a modified Czerny-Turner spectral system. A beam splitter was used to split the spectral coverage into two parts: the first order spectrum ranges from 1 200 nm to 2 400 nm and the second order spectrum ranges from 600 nm to 1 200 nm. Two linear array detectors were used to get the whole spectrum at the same time for a direct-reading spectrum. The dimension of the optical system was about 80 mm55 mm20 mm. After the optimization, the tangential aberration of all the wavelengths was smaller than 6 um. The Spectral Response Function(SRF) was simulated based on the Point Spread Function(PSF) which obtained by direct integration of Huygens wavelets method. The spectral resolution is superior to 2nm from 600nm to 1200nm and 4 nm from 1 200 nm to 2 400 nm by analyzing the spectral bandwidth. The structure of the system is simple and compact with a stable performance. The instrument is applied to the measurement of SSI on the satellite.
- solar spectrograph /
- dichroic beam splitter /
- point spread function(PSF) /
- spectral response function(SRF)

[1]	Wu Lianghai, Gao Jun, Fan Zhiguo, et al. Scattering of particles in the atmosphere and their influence on celestial polarization patterns [J]. Acta Optica Sinica, 2011, 31 (7): 0701005. (in Chnese) 吴良海, 高隽, 范之国, 等. 大气粒子散射特性及其对空间偏振分布的影响[J]. 光学学报, 2011, 31(7): 0701005.
[2]
[3]
[4]	Haigh J D. CLIMATE:climate variability and the influence of the sun[J]. Science, 2001, 294(5549): 2109-2111.
[5]
[6]	Rind D. The sun's role in climate variations [J]. Science, 2002, 296(5568): 673-677.
[7]
[8]	Haigh J D. The impact of solar variability on climate [J]. Science, 1996, 272(5264): 981-984.
[9]
[10]	Rottman G, Mount G, Lawrence G, et al. Solar spectral irradiance measurements: visible to near-infrared regions [J]. Metrologia, 1998, 35(4): 707-712.
[11]
[12]	Thuillier G, Herse M, Labs D, et al. The solar spectral irradiance from 200-2400 nm as measured by the SOLSPEC spectrometer from the ATLAS and EURECA missions [J]. Solar Phys, 2003, 214(1): 1-22.
[13]	Boversmann H, Burrows J, Buchwitz M, et al. SCIAMACHY: mission objectives and measurement modes [J]. J Atmospheric Sciences, 1999, 56(2): 127-150.
[14]
[15]	Harder J, Lawrence G, Rottman G, et al. The spectral irradiance monitor (SIM) for the SORCE mission[C]//SPIE, 2000, 4135: 204.
[16]
[17]
[18]	Zhang Hao, Fang Wei, Ye Xin, et al. Design of prism spectrometer with wide spectral coverage for solar spectrum measurement[J]. Acta Optica Sinica, 2013, 33(2): 0222001. (in Chnese) 张浩, 方伟, 叶新, 等. 宽光谱棱镜型太阳光谱仪设计[J]. 光学学报, 2013, 33(2): 0222001.
[19]
[20]	Xue Qingsheng, Chen Wei. Design of modified Czerny- Turner spectral imaging system with wide spectral region[J]. Optics and Precision Engineering, 2012, 20(2): 233-240. (in Chnese) 薛庆生, 陈伟. 改进的宽谱段车尔尼-特纳光谱成像系统设计[J]. 光学精密工程, 2012, 20(2): 233-240.
[21]
[22]	Cheng Xin, Zhang Bao, Hong Yongfeng, et al. Optical design of an airborne dual-wavelength imaging spectrometer with high throughput [J]. Infrared and Laser Eng, 2012, 41 (3): 690-695. (in Chnese) 程欣, 张葆, 洪永丰, 等. 机载高光通量双波段成像光谱仪的设计[J]. 红外与激光工程, 2012, 41(3): 690-695.
[23]
[24]	Green R O. Spectral calibration requirement for earth-looking imaging spectrometers in the solar-reflected spectrum [J]. Applied Optics, 1998, 37(4): 683-690.
[25]	Mouroulis P, Green R O, Chrien T G. Design of pushbroom imaging spectrometers for optimum recovery of spectroscopic and spatial information [J]. Applied Optics, 2000, 39 (13): 2210-2220.

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小型宽光谱太阳光谱仪光学设计

1. 中国科学院长春光学精密机械与物理研究所,吉林长春130033;

2. 中国科学院大学,北京100049

作者简介:
高震宇(1988-),男,博士生,主要从事空间光谱仪器光学设计方面的研究。Email:lnsygzy92@zju.edu.cn

收稿日期: 2014-06-10
修回日期: 2014-07-15
刊出日期: 2015-02-25

基金项目:

国家自然科学基金(41227003)

中图分类号: O433;TH744

关键词:

摘要: 针对大气层外的太阳光谱辐照度监测,设计了一种星载小型宽光谱太阳光谱仪。光学系统应用改进的切尔尼-特纳光学结构,工作波长范围为600~1 200 nm(二级光谱)和1 200~2 400 nm(一级光谱);一二级光谱使用二向色分光镜分离,并采用两片线阵探测器同时接收,实现全谱瞬态直读。整个光学结构的尺寸为80 mm55 mm20 mm。经过系统优化,全谱段子午方向像差低于6 m。基于惠更斯点扩散函数(PSF),仿真探测器像元的光谱响应函数(SRF),结果表明光谱分辨率在600~1 200 nm波段优于2 nm,在1 200~2 400 nm波段优于4 nm。系统结构简单紧凑,稳定性高,适合用于空间太阳光谱辐照度的在轨监测。

English Abstract

Design of a small-size solar spectrograph with wide spectral range

1. Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences,Changchun 130033,China;

2. University of Chinese Academy of Sciences,Beijing 100049,China

Received Date: 2014-06-10
Rev Recd Date: 2014-07-15
Publish Date: 2015-02-25

Keywords:

Abstract: A small-size satellite-borne solar spectrograph with wide spectral range was designed to monitor the Solar Spectral Irradiance (SSI) outside the atmosphere. The instrument used a modified Czerny-Turner spectral system. A beam splitter was used to split the spectral coverage into two parts: the first order spectrum ranges from 1 200 nm to 2 400 nm and the second order spectrum ranges from 600 nm to 1 200 nm. Two linear array detectors were used to get the whole spectrum at the same time for a direct-reading spectrum. The dimension of the optical system was about 80 mm55 mm20 mm. After the optimization, the tangential aberration of all the wavelengths was smaller than 6 um. The Spectral Response Function(SRF) was simulated based on the Point Spread Function(PSF) which obtained by direct integration of Huygens wavelets method. The spectral resolution is superior to 2nm from 600nm to 1200nm and 4 nm from 1 200 nm to 2 400 nm by analyzing the spectral bandwidth. The structure of the system is simple and compact with a stable performance. The instrument is applied to the measurement of SSI on the satellite.