Chinese Journal of Lasers, Volume. 45, Issue 9, 911007(2018)

Review on Noise Immune Cavity Enhanced Optical Heterodyne Molecular Spectroscopy

Ma Weiguang1,2, Zhou Yueting1,2, Zhao Gang1,2, Jia Mengyuan1,2, Liu Jianxin1,2, Guo Songjie1,2, Dong Lei1,2, Zhang Lei1,2, Yin Wangbao1,2, Xiao Liantuan1,2, Axner Ove3, and Jia Suotang1,2
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3Department of Physics, Ume University, Ume Sweden, SE-901 87
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    Figures & Tables(8)
    (a) Principle of NICE-OHMS; relationship of laser components and cavity modes when cavity is (b) empty or (c) filled with targeted gas
    Experimental setup of NICE-OHMS based on EDFL
    Doppler broadened (a) absorption and (b) dispersion NICE-OHMS signals
    Development of detection sensitivity based on Doppler broadened NICE-OHMS
    Effects of same loss and different precision on NICE-OHMS signal
    (a) CEAS and (b) NICE-OHMS signals with frequency locking by controlling PZT; (c) CEAS and (d) NICE-OHMS signals with frequency locking by controlling combination of PZT and AOM
    Schematic of (a) differential and (b) balanced detected NICE-OHMS
    • Table 1. Some important parameters of NICE-OHMS performed by research groups so far

      View table

      Table 1. Some important parameters of NICE-OHMS performed by research groups so far

      ReferenceLaserFinesseWavelength /nmTargeted gasDetectionSensitivity /cm-1Detection mode
      Ref. [40] 1996Nd∶YAG93001064C2HD1.8×10-12sD
      Ref. [16] 1998Nd∶YAG1000001064C2HD1.4×10-14sD
      Ref.[28] 1999Ti∶sapphire17000790C2HD1.4×10-14sD
      Ref. [33] 1999ECDL3001660CH49.5×10-11sD
      Ref. [12] 1999ECDL6000763O23.8×10-11DB
      Ref.[41] 2002Ti∶sapphire16400818C2H26×10-12DB
      Ref.[34] 2004QCL24158518N2O9.7×10-11DB
      Ref. [42] 2004ECDL11000771O27×10-12DB
      Ref.[43] 2006Ti∶sapphire20700797NO2×10-10DB
      Ref.[44] 2007EDFL48001531C2H28×10-11DB/sD
      Ref.[22] 2009ECDL26001513CH42×10-11DB
      Ref.[36] 2010DFB4601551C2H22×10-10DB
      Ref. [20] 2010Ti∶sapphire300924N2+DB
      Ref.[45] 2012ECDL48001510HO21.8×10-9DB
      Ref.[35] 2012DFG3002800-4800CH42×10-7DB
      Ref. [38] 2014OPO1503200-3900HeH+, H3+,HCO+ CH5+DB
      Ref.[21] 2015ECDL16001529CH4,C2H2,HCN4.6×10-8DB
      Ref.[23] 2015QD-ECDL89701283N2O6×10-9DB
      Ref.[46] 2015ECDL185001400HD9.2×10-9sD
      Ref.[18] 2015EDFL550001531C2H22.2×10-13DB
      Ref.[47] 2016OPO1303100HNO+1×10-9DB
      Ref.[39] 2017WGM550001536C2H2, CO26.6×10-14DB
      Ref.[37] 2017DFB1690001532CH41×10-10DB
      Ref.[48] 2017EDFL550001531C2H24.7×10-14DB
      Ref.[19] 2018EDFL550001531C2H22.2×10-14DB
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    Ma Weiguang, Zhou Yueting, Zhao Gang, Jia Mengyuan, Liu Jianxin, Guo Songjie, Dong Lei, Zhang Lei, Yin Wangbao, Xiao Liantuan, Axner Ove, Jia Suotang. Review on Noise Immune Cavity Enhanced Optical Heterodyne Molecular Spectroscopy[J]. Chinese Journal of Lasers, 2018, 45(9): 911007

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    Paper Information

    Special Issue:

    Received: Apr. 3, 2018

    Accepted: --

    Published Online: Sep. 8, 2018

    The Author Email:

    DOI:10.3788/CJL201845.0911007

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