Spectroscopy and Spectral Analysis, Volume. 41, Issue 12, 3892(2021)

Solar Radiation Observation During a Solar Eclipse in Tibet

Qian WANG, Gelsor Norsang*;, Wangmu Tsoja, Tunzhup Lagba, Dopwang Pu, Juan LIU, Yi ZHOU, and Xi ZE
Author Affiliations
  • Solar UV Lab, Tibet University, Lhasa 850000, China
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    Figures & Tables(15)
    Real sky pictures of the Lhasa solar eclipse on June 21, 2020, in Lhasa, Tibet
    Real sky pictures of the golden edge annular eclipse on June 21, 2020, in Ngari, Tibet
    (a) Lhasa spectrometers; (b) Lhasa Pyranometer; (c) Ngari observation site
    Three dimensional spectral characteristics for the solar eclipse on June 21, 2020 in Singgekapap, Ngari, Tibet
    Three dimensional spectral characteristics for clear sky on June 22, 2020 in Singgekapap, Ngari, Tibet
    Three dimensional spectral characteristics of the solar eclipse on June 21, 2020 in Lhasa
    Three dimensional spectral features of quasi-clear sky on June 26, 2020 in Lhasa
    Spectral variation during the annular eclipse in Ngari
    Spectral features during annular solar eclipse in Lhasa
    Global solar irradiance for the annular eclipse in Ngari
    Global solar irradiance for the annular eclipse in Lhasa
    Solar UVB for the solar eclipse in Lhasa
    • Table 1. Information of the solar eclipse on June 21, 2020 and its observation sites in Tibet

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      Table 1. Information of the solar eclipse on June 21, 2020 and its observation sites in Tibet

      SiteLocal
      noon
      Altitude
      /m
      Longitude/
      latitude
      Magnitude
      of eclipse
      First
      contact
      phase
      Maximum
      phase
      Last
      contact
      phase
      Duration
      of the
      eclipse
      Weather
      Gnari14:414 30080°5'45″E
      32°30'22″N
      0.99513:00:5914:44:1416:28:2503:27:26Partial clouds
      Lhasa13:573 68591°10'40″E
      29°38'48″N
      0.95313:26:4415:13:0916:50:4203:23:58Partial clouds
    • Table 2. Peak variations of the strongest monochromatic light for the solar eclipse in Ngari

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      Table 2. Peak variations of the strongest monochromatic light for the solar eclipse in Ngari

      日食过程波长
      /nm
      单色光强峰值
      /(mW·m-2)
      初亏(13:01)1 669.234
      食甚(14:41)476.1361.936
      复圆(16:28)1 522.388
    • Table 3. Peak variations of the strongest monochromatic light for the solar eclipse in Lhasa

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      Table 3. Peak variations of the strongest monochromatic light for the solar eclipse in Lhasa

      日食过程波长
      /nm
      单色光强峰值
      /(mW·m-2)
      初亏(13:27)1 563.876
      食甚(15:13)476.6126.391
      复圆(16:51)735.191
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    Qian WANG, Gelsor Norsang, Wangmu Tsoja, Tunzhup Lagba, Dopwang Pu, Juan LIU, Yi ZHOU, Xi ZE. Solar Radiation Observation During a Solar Eclipse in Tibet[J]. Spectroscopy and Spectral Analysis, 2021, 41(12): 3892

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    Paper Information

    Category: Research Articles

    Received: Nov. 19, 2020

    Accepted: --

    Published Online: Dec. 17, 2021

    The Author Email:

    DOI:10.3964/j.issn.1000-0593(2021)12-3892-09

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