• Chinese Optics Letters
  • Vol. 13, Issue Suppl., S21413 (2015)
Hui Lan1、3, Xinbing Wang2、*, Hong Chen1, Duluo Zuo2, and Peixiang Lu2
Author Affiliations
  • 1School of Optical and Electronic Information, Huazhong University of Science and Technology, Wuhan 430074, China
  • 2Wuhan National Laboratory for Optoelectronics, Huazhong University of Science and Technology, Wuhan 430074, China
  • 3School of Physics and Information Engineering, Jianghan University, Wuhan 430056, China
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    DOI: 10.3788/COL201513.S21413 Cite this Article Set citation alerts
    Hui Lan, Xinbing Wang, Hong Chen, Duluo Zuo, Peixiang Lu. Temporal evolution of Nd:YAG laser-produced Sn plasma[J]. Chinese Optics Letters, 2015, 13(Suppl.): S21413 Copy Citation Text show less
    Schematic of the experimental setup used for ICCD imaging and OES of a Nd:YAG laser-produced Sn plasma.
    Fig. 1. Schematic of the experimental setup used for ICCD imaging and OES of a Nd:YAG laser-produced Sn plasma.
    EUV and laser waveform in an oscilloscope.
    Fig. 2. EUV and laser waveform in an oscilloscope.
    Time evolution of Sn plasma expansion and the emission spectrum with an air pressure of 50 Pa and laser energy of 130 mJ.
    Fig. 3. Time evolution of Sn plasma expansion and the emission spectrum with an air pressure of 50 Pa and laser energy of 130 mJ.
    Particle kinetic energy versus delay time along the normal to the target surface at 50 Pa and laser energy of 130 mJ.
    Fig. 4. Particle kinetic energy versus delay time along the normal to the target surface at 50 Pa and laser energy of 130 mJ.
    Temporal evolution of the Sn I 510.46 nm and Sn II 533.23 nm line at the delay time from 38 ns to 143 ns.
    Fig. 5. Temporal evolution of the Sn I 510.46 nm and Sn II 533.23 nm line at the delay time from 38 ns to 143 ns.
    Temporal evolution of the electron temperature and density.
    Fig. 6. Temporal evolution of the electron temperature and density.
    Maximum kinetic energy versus the delay time under different atmosphere pressure and laser energy, respectively.
    Fig. 7. Maximum kinetic energy versus the delay time under different atmosphere pressure and laser energy, respectively.
    Variation of maximum electron temperature and electron density with delay time under different pressures (5 Pa, 50 Pa, 102 Pa, 103 Pa, 104 Pa).The incident energy is 130 mJ.
    Fig. 8. Variation of maximum electron temperature and electron density with delay time under different pressures (5 Pa, 50 Pa, 102Pa, 103Pa, 104Pa).The incident energy is 130 mJ.
    Variation of maximum electron temperature and electron density for different incident laser energies (50, 104, 130, 182 mJ). The air pressure is 50 Pa.
    Fig. 9. Variation of maximum electron temperature and electron density for different incident laser energies (50, 104, 130, 182 mJ). The air pressure is 50 Pa.
    Hui Lan, Xinbing Wang, Hong Chen, Duluo Zuo, Peixiang Lu. Temporal evolution of Nd:YAG laser-produced Sn plasma[J]. Chinese Optics Letters, 2015, 13(Suppl.): S21413
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