Volume 45 Issue 12
Jan.  2017
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Dai Congming, Zhang Zhiyong, Ma Li, Feng Zhiwei, Wei Heli. Measuring and analysis of atmospheric transfer and environment background character on infrared telescope site[J]. Infrared and Laser Engineering, 2016, 45(12): 1204005-1204005(7). doi: 10.3788/IRLA201645.1204005
Citation: Dai Congming, Zhang Zhiyong, Ma Li, Feng Zhiwei, Wei Heli. Measuring and analysis of atmospheric transfer and environment background character on infrared telescope site[J]. Infrared and Laser Engineering, 2016, 45(12): 1204005-1204005(7). doi: 10.3788/IRLA201645.1204005

Measuring and analysis of atmospheric transfer and environment background character on infrared telescope site

doi: 10.3788/IRLA201645.1204005
  • Received Date: 2016-04-10
  • Rev Recd Date: 2016-05-20
  • Publish Date: 2016-12-25
  • Selecting a fine atmospheric site is very important for ground-based infrared astronomy. The sky background radiance and atmospheric transmittance are important factors for selecting site. Combined observations of solar spectral extinction and forward angular scattering were presented with ground-based FTIR on Yangbajing, Tibet. The direct solar irradiance and atmospheric background radiance were showed on 8-14 m band. According to the atmospheric parameters, the direct solar radiance, atmospheric spectral transmittance and background radiance of selecting sites were compared by CART on long-wave infrared band. These will be useful to select a site for ground-based infrared solar telescope.
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    [2] Qian Xuan, Wang Panxing, Yao Yongqiang, et al. Time variation of astro-climate conditions in China[J]. Sci Sin Phys Mech Astron, 2011, 41(7):896-910. (in Chinese)钱璇,王盘兴,姚永强,等.中国天文气象特征的时变特征[J]. 中国科学物理学:力学天文学, 2011, 41(7):896-910.
    [3] Wu Xiaoqing. Site testing for ground-based optical telescope[J]. Journal of Anhui Normal University(Natural Science), 2013, 36(5):414-418. (in Chinese)吴晓庆.地基天文光学望远镜选址[J]. 安徽师范大学学报(自然科学版), 2013, 36(5):414-418.
    [4] Liu Guangqian, Yang Lei, Deng Linhua, et al. Influence of atmospheric turbulence on the accuracy of astronomical telescope auto-guiding system[J]. Acta Optica Sinica, 2013, 33(1):0101002-1-5. (in Chinese)柳光乾, 杨磊, 邓林华, 等. 大气湍流对天文望远镜光电导行精度的影响[J]. 光学学报, 2013, 33(1):0101002-1-5.
    [5] Kenyon S L, Storey J W V. A review of optical sky brightness and extinction at Dome C. Antarctica[J]. Publications of the Astronomical Society of the Pacific, 2006, 118(841):489-502.
    [6] Walden V P, Town M S, Halter B, et al. First measurements of the Infrared Sky Brightness at Dome C, Antarctica[J]. Publications of the Astronomical Society of the Pacific 2005, 117:300-308.
    [7] Evans W F J, Puckrin E. Combined measurements of thermal emission and solar absorption of atmospheric carbon monoxide[J]. Atmospheric Environment, 1993, 33:2081-2088.
    [8] Wei Heli, Chen Xiuhong, Dai Congming, et al. Ground-based measurements of infrared atmospheric background spectral radiances[J]. Infrared and Laser Engineering, 2012, 41(2):284-290. (in Chinese)魏合理, 陈秀红, 戴聪明,等.地基大气背景红外光谱辐射特性测量[J]. 红外与激光工程, 2012, 41(2):284-290.
    [9] Yao Yongqiang. The astronomical site survey in west China[J]. Journal of Korean Astronomical Society, 2005, 39:113-116.
    [10] Gardiner T D, Coleman M, Browning H, et al. Absolute high spectral resolution measurements of surface solar radiation for detection of water vapor continuum absorption[J]. Phil Trans R Soc A, 2012, 370:2590-2610.
    [11] Wei Heli, Chen Xiuhong, Rao Ruizhong. Introduction to the combined atmospheric radiative transfer software CART[J].Journal of Atmospheric and Environmental Optics, 2007, 2(6):446-450. (in Chinese)魏合理, 陈秀红, 饶瑞中. 通用大气辐射传输软件(CART)介绍[J]. 大气与环境光学学报, 2007, 2(6):446-450.
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Measuring and analysis of atmospheric transfer and environment background character on infrared telescope site

doi: 10.3788/IRLA201645.1204005
  • 1. Key Laboratory of Atmospheric Composition and Optical Radiation,Anhui Institute of Optics and Fine Mechanics,Chinese Academy of Sciences,Hefei 230031,China;
  • 2. Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100049,China;
  • 3. School of Environmental Sciences and Optoelectronic Technology,University of Science and Technology of China,Hefei 230031,China

Abstract: Selecting a fine atmospheric site is very important for ground-based infrared astronomy. The sky background radiance and atmospheric transmittance are important factors for selecting site. Combined observations of solar spectral extinction and forward angular scattering were presented with ground-based FTIR on Yangbajing, Tibet. The direct solar irradiance and atmospheric background radiance were showed on 8-14 m band. According to the atmospheric parameters, the direct solar radiance, atmospheric spectral transmittance and background radiance of selecting sites were compared by CART on long-wave infrared band. These will be useful to select a site for ground-based infrared solar telescope.

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