| 北京天文台兴隆观测站夜天光光谱证认 |
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| 引用本文： | 姜晓军,姜晓军,徐达维,胡景耀,胡景耀.北京天文台兴隆观测站夜天光光谱证认[J].中国天文和天体物理学报,1999(2). |
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| 作者姓名： | 姜晓军 姜晓军 徐达维 胡景耀 胡景耀 |
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| 作者单位： | 国科学院北京天文台!北京１０００８０(姜晓军，徐达维，胡景耀)，中国科学院光学天文联合实验室!上海２０００３０(姜晓军，胡景耀) |
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| 摘 要： | 介绍了夜天光光谱的观测方法，给出了北京天文台兴隆观测站５３０ｎｍ－８２０ｎｍ的夜天光发射光谱，并对它们进行了证认，测定了大气辉光线的夜变化；光谱中城市灯光线ＮａＩ和ＨｇＩ均较弱，表明兴隆站目前的光污染尚不严重．
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| 关 键 词： | 夜天光光谱 证认 大气辉光线 |
Identification of the Night Sky Spectra of Xinglong Station, Beijing Astronomical Observatory |
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| JIANG Xiao-jun, XU Da-wei, HU Jing-yao.Identification of the Night Sky Spectra of Xinglong Station, Beijing Astronomical Observatory[J].Chinese Journal of Astronomy and Astrophysics,1999(2). |
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| Authors: | JIANG Xiao-jun XU Da-wei HU Jing-yao |
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| Institution: | JIANG Xiao-jun,1,2 XU Da-wei,1 HU Jing-yao1,21 |
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| Abstract: | e identified the night sky emission lines from 5300 to 8200 Angstrom at XinglongStation, Beijing Astronomical Observatory, and measured the variations of airglow emissionlines during one night. The Nal and HgI lines from city lights are quite weak, which meanslight pollution is not serious yet at Xinglong Station. |
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| Keywords: | night sky spectra --identification-airglow emission lines |
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