CHA Guang-wei. Parameter Determination and Fe-Ar Calibration Spectrum Identification for the Coude Spectrograph-CCD System of the 1m Telescope at Yunnan Observatory[J]. Publications of the Yunnan Observatory, 2001, (3): 1-120.
Citation: CHA Guang-wei. Parameter Determination and Fe-Ar Calibration Spectrum Identification for the Coude Spectrograph-CCD System of the 1m Telescope at Yunnan Observatory[J]. Publications of the Yunnan Observatory, 2001, (3): 1-120.

Parameter Determination and Fe-Ar Calibration Spectrum Identification for the Coude Spectrograph-CCD System of the 1m Telescope at Yunnan Observatory

More Information
  • Received Date: October 18, 2000
  • Published Date: July 14, 2001
  • Related parameters of the Coude spectrograph-CCD system and identifications of Fe-Ar emission spectra in the CCD corresponding region are given in this paper for the 1M telescope at Yunnan Observatory. It is found that the chromatic dispersion of the Coude system is almost flat. Dispersions in grade 1-3 are 8.391ű0.09Å/mm(m=1), 4.185ű0.05Å/mm(m=2) and 2.794ű0.03Å/mm(m=3) respectively. The identification chart of the Fe-Ar spectra contains standard emission line from 3370 to 11150Å. The wavelength table listed and the chards shown can be used for the wavelength calibration of program objects.
  • Relative Articles

    [1]Lu Yangping, Le Guiming, Zhao Haofeng, Yin Zhiqiang. The Relationship between First X-Class Flare, First High Latitude Sunspot Hemisphere Features and the Asymmetry of Solar Activity during Solar Cycle 21-24[J]. Astronomical Research and Technology, 2016, 13(2): 150-152.
    [2]Xu Zhi, Yang Lei, Xiang Yongyan, Zheng Yanfang, Mao Weijun, Jin Zhenyu. An Investigation of Spectral-Line Profiles from the Wavelength- Scanning with a Narrow-Band Hα Lyot Filter on the YNAO New Vacuum Solar Telescope[J]. Astronomical Research and Technology, 2014, 11(3): 239-246.
    [3]Yang Yunfei, Feng Song, Ji Kaifan. An Evaluation of the Performance of the 4K×4K CCD on the YNAO Full-Disk Hα Telescope for Solar Observations[J]. Astronomical Research and Technology, 2014, 11(1): 60-64.
    [4]Zhao Shiqing, Li Qiongying, Feng Yongli, Ma Kaiquan, Lin Jun, Wu Mingchan. Observations of the Venus Transit across the Solar Hα Chromosphere in June 6, 2012[J]. Astronomical Research and Technology, 2013, 10(3): 214-218.
    [5]ZHAO Shi-qing, LI Qiong-ying, CHEN Hua-dong, MA Su-li, LI Le-ping, JIANG Yun-chun, WU Ming-chan. Hα Chromospheric Observations of the Venus Transit on June 8, 2004[J]. Astronomical Research and Technology, 2004, 1(3): 241-245.
    [6]ZHANG Heng, LUAN Di. Reconnecting and Evaporating Flare Model Observed in the Flare of AR7186 of 1992 June 4[J]. Publications of the Yunnan Observatory, 1999, 0(4): 1-18.
    [7]Ma Yuan, Xia Zhiguo. The Correlation Analysis On the Solar Radiation Events and Hα Flares[J]. Publications of the Yunnan Observatory, 1995, 0(4): 6-9.
    [8]Jin Xing YAO. EVIDENCE FOR STOCHASTIC ELECTRON ACCELERATION IN THE CM2 COMPONENT OF 1988 JUNE FLARES[J]. Publications of the Yunnan Observatory, 1989, 0(S1): 130-134.
    [9]Zu Yan ZHU. THE POSTFLARE LOOP OF THE 2B FLARE ON JAN.14, 1989[J]. Publications of the Yunnan Observatory, 1989, 0(S1): 114-116.
    [10]Hong Zhao WANG, Ti LUAN. The rapid development and frequently-occurring X class x-ray flares in AR5047[J]. Publications of the Yunnan Observatory, 1989, 0(S1): 52-56.

Catalog

    Article views (117) PDF downloads (10) Cited by()

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return