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抚仙湖一米新真空太阳望远镜6米近红外光谱仪装调及太阳1.56微米光谱的初步观测结果
Installation/Adjustment of a 6m Near-Infrared Spectrograph for the lm New Vacuum Solar Telescope in the Fuxian-Lake Solar-Observation Station and Preliminary Observation Results of Solar Spectra around 1.56μm Using the Spectrograph

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文摘 主要介绍了抚仙湖1m新真空太阳望远镜(the 1-meter New Vacuum Solar Telescope,NVST)6m水平式近红外光谱仪的安装过程和实测结果。主要讨论内容是光路设计特点、光学系统的装调以及利用该光谱仪对活动区NOAA 11662黑子进行的初步近红外光谱实测(波长1.56 μm附近)。成功观测到由黑子强磁场造成的Fe I 1.56 μm谱线裂变现象,并初步估算了磁场强度。该光谱的成功装调和使用,充分实现了对9m光谱仪光学系统的整体检测,为9 m光谱仪的安装调试提供了宝贵的经验和参考。
其他语种文摘 This paper first presents the design, layout, and installation of a near-infrared grating spectrograph installed on the 1m new vacuum solar telescope in the Fuxian-Lake Solar-Observation Station of the Yunnan Observatories. It records spectra in the wavelength range of 1.0μm-2.0μm. The focal length of its collimating mirror is 6m and its spectral resolution can reach about 6x 10~(-6)μm/pixel. Using this spectrograph and a previously built near-infrared detector (with an InGaAs detector of 512x640 pixels and a pixel size of 25 μm) we can obtain solar spectra with a wavelength coverage of 0. 004μm. One purpose of making this horizontal-type spectrograph is to evaluate main designs to be used in the vertical-type 9m near-infrared spectrograph in future. The designs include those of the Echelle grating, infrared detector, and infrared front-filter. With the spectrograph we can also accumulate experience of observing near-infrared solar spectra, particularly, in setting the slit width, exposure time, and wavelength calibration. Using the spectrograph we successfully observed a sunspot region in a wavelength range around 1.565 μm. This range covers two commonly studied spectral lines (Fe I 1.5648μm and Fe I 1.5653μm),which are sensitive to solar magnetic-field strengths. We reduced the data using codes designed for the 1m telescope. The wavelength calibration is based on the standard solar spectrum. We calculated the magnetic-field strength (instead of the magnetic-field flux) from the line split rather straightforwardly. These preliminary results demonstrate the effectiveness of this 6m spectrograph in achieving its scientific goals.
来源 天文研究与技术 ,2014,11(2):168-175 【扩展库】
关键词 光谱仪 ; 近红外 ; 抚仙湖1 m新真空太阳望远镜
地址

中国科学院云南天文台, 云南, 昆明, 650011

语种 中文
文献类型 研究性论文
ISSN 1672-7673
学科 天文学
基金 国家自然科学基金 ;  西部之光项目“抚仙湖一米红外太阳塔红外大色散光谱仪研制” ;  物质科学前沿与交叉研究II “红外太阳物理”
文献收藏号 CSCD:5112464

参考文献 共 5 共1页

1.  Wang R. The first observation and data reduction of the Multi-wavelength Spectrometer on the New Vacuum Solar Telescope. Research in Astronomy and Astrophysics,2013,13(10):1240-1254 CSCD被引 23    
2.  Li H. Two-dimensional He I 10830A spectroscopy of a subflare. Chinese Astronomy and Astrophysics,1995,20(1):85-91 CSCD被引 1    
3.  何剑. PtSi IRCCD像机对红外太阳光谱的观测. 半导体光电,2000,21(S1):62-66 CSCD被引 1    
4.  曹文达. 太阳光谱仪用探测器的研究. 天文学报,2000,41(1):93-103 CSCD被引 1    
5.  Litzen U. The Fe I spectrum in the region 1-4μm. Physica Scripta,1976,13(4):240-244 CSCD被引 1    
引证文献 3

1 韩笑 一米新真空太阳望远镜多波段光谱仪CaⅡ通道杂散光研究 天文研究与技术,2016,13(4):446-454
CSCD被引 1

2 韩笑 一米新真空太阳望远镜多波段光谱仪杂散光及空间PSF的测量 天文研究与技术,2017,14(1):52-59
CSCD被引 2

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