• High Power Laser Science and Engineering
  • Vol. 4, Issue 3, 03000e27 (2016)
Fei-Lu Wang1, Xiao-Xing Pei1、2, Bo Han1、2, Hui-Gang Wei1, Da-Wei Yuan1, Gui-Yun Liang1, Gang Zhao1、2, Jia-Yong Zhong3, Zhe Zhang4, Bao-Jun Zhu2、4, Yan-Fei Li2、4, Fang Li4, Yu-Tong Li2、4, Si-Liang Zeng5, Shi-Yang Zou5, and Jie Zhang6
Author Affiliations
  • 1Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • 3Department of Astronomy, Beijing Normal University, Beijing 100875, China
  • 4Beijing National Laboratory of Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 5Institute of Applied Physics and Computational Mathematics, Beijing, 100088, China
  • 6Shanghai Jiao Tong University, Shanghai 200240, China
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    DOI: 10.1017/hpl.2016.27 Cite this Article Set citation alerts
    Fei-Lu Wang, Xiao-Xing Pei, Bo Han, Hui-Gang Wei, Da-Wei Yuan, Gui-Yun Liang, Gang Zhao, Jia-Yong Zhong, Zhe Zhang, Bao-Jun Zhu, Yan-Fei Li, Fang Li, Yu-Tong Li, Si-Liang Zeng, Shi-Yang Zou, Jie Zhang. Laboratory astrophysics with laser-driven strong magnetic fields in China[J]. High Power Laser Science and Engineering, 2016, 4(3): 03000e27 Copy Citation Text show less
    Schematic view of the experimental setup at the Shenguang-II laser facility. Eight laser beams at 351 nm were divided into two bunches and focused onto both sides of the planar plate simultaneously.
    Fig. 1. Schematic view of the experimental setup at the Shenguang-II laser facility. Eight laser beams at 351 nm were divided into two bunches and focused onto both sides of the planar plate simultaneously.
    (a) Shows a cartoon simulating the solar flares and the coupling of solar wind with earth magnetosphere. (b) MR model for the loop-top x-ray source, x-ray images taken with Pinhole camera in the experiment. (c) MR model for the interaction of solar wind with magnetosphere, one micro-solar-flare is produced by two intense laser beams interacting with a solid aluminum block, and the outflow interacts with a preset permanent magnetic pole.
    Fig. 2. (a) Shows a cartoon simulating the solar flares and the coupling of solar wind with earth magnetosphere. (b) MR model for the loop-top x-ray source, x-ray images taken with Pinhole camera in the experiment. (c) MR model for the interaction of solar wind with magnetosphere, one micro-solar-flare is produced by two intense laser beams interacting with a solid aluminum block, and the outflow interacts with a preset permanent magnetic pole.
    Unfolded spectrum of the descending edge of the main peak of X0115$+$63[2].
    Fig. 3. Unfolded spectrum of the descending edge of the main peak of X0115$+$63[2].
    WavelengthMethodMagnetic-field strength at the B-dotCurrent
    (J)(nm)()(T)(mA)(T)
    536.24351$1.87\times 10^{14}$B-dot0.00650.04445
    1004.27351$3.50\times 10^{14}$B-dot0.0110.07173
    1780.4351$6.21\times 10^{14}$B-dot0.160.10102
    1966.8351$6.85\times 10^{14}$B-dot0.0310.20205
    Table 1. Summary of magnetic-field strength, and current in the coil.
    Fei-Lu Wang, Xiao-Xing Pei, Bo Han, Hui-Gang Wei, Da-Wei Yuan, Gui-Yun Liang, Gang Zhao, Jia-Yong Zhong, Zhe Zhang, Bao-Jun Zhu, Yan-Fei Li, Fang Li, Yu-Tong Li, Si-Liang Zeng, Shi-Yang Zou, Jie Zhang. Laboratory astrophysics with laser-driven strong magnetic fields in China[J]. High Power Laser Science and Engineering, 2016, 4(3): 03000e27
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