• Chinese Journal of Lasers
  • Vol. 51, Issue 7, 0701011 (2024)
Kui Li1、4, Runyu Meng2、3, Ruixuan Li1、4, Guangyin Zhang1、4, Mingjie Yao5, Hao Xu1, Yutong Wang1, Jie Li1、4、***, Xiaoshi Zhang1、2、**, and Zhongwei Fan4、*
Author Affiliations
  • 1Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100094, China
  • 2School of Physics and Astronomy, Yunnan University, Kunming 650216, Yunnan, China
  • 3Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, Yunnan, China
  • 4School of Optoelectronics, University of Chinese Academy of Sciences, Beijing 100049, China
  • 5School of Instrumentation and Optoelectronic Engineering, Beihang University, Beijing 100191,China
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    DOI: 10.3788/CJL231507 Cite this Article Set citation alerts
    Kui Li, Runyu Meng, Ruixuan Li, Guangyin Zhang, Mingjie Yao, Hao Xu, Yutong Wang, Jie Li, Xiaoshi Zhang, Zhongwei Fan. High Power and High Stability 13.5 nm Extreme Ultraviolet Light Source Driven by High‑Order Harmonics[J]. Chinese Journal of Lasers, 2024, 51(7): 0701011 Copy Citation Text show less
    Schematics of experimental setup. (a) Ti∶sapphire light source system; (b) beam stability control system; (c) EUV generation and filtration system; (d) EUV light source detection and spectrometer system
    Fig. 1. Schematics of experimental setup. (a) Ti∶sapphire light source system; (b) beam stability control system; (c) EUV generation and filtration system; (d) EUV light source detection and spectrometer system
    Schematics of high-order harmonic optical power measurement. (a) EUV light power measurement system and pointing stability measurement system; (b) harmonic spot collected at 1.9 m from light source
    Fig. 2. Schematics of high-order harmonic optical power measurement. (a) EUV light power measurement system and pointing stability measurement system; (b) harmonic spot collected at 1.9 m from light source
    Power stability and pointing stability test results. (a) Average power curve of beam within 12 h; (b) coordinate of center of HHG spot collected by CMOS
    Fig. 3. Power stability and pointing stability test results. (a) Average power curve of beam within 12 h; (b) coordinate of center of HHG spot collected by CMOS
    Results of spectral acquisition and analysis. (a) Schematic of spectral acquisition device; (b) spectral calibration analysis results of gratings with groove density of 500 line/mm
    Fig. 4. Results of spectral acquisition and analysis. (a) Schematic of spectral acquisition device; (b) spectral calibration analysis results of gratings with groove density of 500 line/mm
    Grating spectral results. (a) First-order spectral information collected by CMOS; (b) extracted first-order spectral information
    Fig. 5. Grating spectral results. (a) First-order spectral information collected by CMOS; (b) extracted first-order spectral information
    HHG spectral distributions acquired by grating with groove density of 500 line/mm. (a) Theoretical absolute grating efficiency; (b) harmonic spectra obtained from measurement
    Fig. 6. HHG spectral distributions acquired by grating with groove density of 500 line/mm. (a) Theoretical absolute grating efficiency; (b) harmonic spectra obtained from measurement
    Kui Li, Runyu Meng, Ruixuan Li, Guangyin Zhang, Mingjie Yao, Hao Xu, Yutong Wang, Jie Li, Xiaoshi Zhang, Zhongwei Fan. High Power and High Stability 13.5 nm Extreme Ultraviolet Light Source Driven by High‑Order Harmonics[J]. Chinese Journal of Lasers, 2024, 51(7): 0701011
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