Matter and Radiation at Extremes, Volume. 10, Issue 3, 037401(2025)

Magnetic transport and radiation properties during compression of a magnetized plasma

Zhao Wang1,2, Rui Cheng1,2,3, Xuejian Jin1,2, Yanhong Chen1, Lulin Shi1,4, Guodong Wang1,2, Zexian Zhou1,4, Zakir Iqbal1,2, Yupeng Chen1, Jinfu Zhang3, Xiaoxia Wu1, Yu Lei1, Yuyu Wang1,2,3, Yongtao Zhao5, Shuai Liu5, Liangwen Chen1,2,3, and Jie Yang1,2,3
Author Affiliations
  • 1Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • 3Advanced Energy Science and Technology Guangdong Laboratory, Huizhou 516003, China
  • 4College of Physics and Electronic Engineering, Northwest Normal University, Lanzhou 730070, China
  • 5Xi’an Jiaotong University, Xi’an 710049, China
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    Figures & Tables(7)
    Schematic of experimental setup. A detailed description of all settings can be found in the text. It is important to note that photodiode-1 measures the luminosity in both the vessel and the right-side extension tube, while photodiode-2 measures only the luminosity in the left-side extension tube, aiming to monitor when the plasma begins to eject axially.
    Temporal profiles of drive current (light salmon pink), magnetic field (purple), and luminosity (rose), measured at 20 Pa and 20 kV, with a time resolution of 0.01 μs.
    Observation of bulk plasma motion. (a) Time-series images of magnetized plasma implosion within the second half-cycle of the pinch. The exposure time for each frame is 15 ns. (b) Time variation of the radius of the outer boundary of the plasma column, as extracted from (a). The curve is included to guide the eyes.
    Time-dependent plasma density and temperature. Stage-1 and Stage-2 refer to the last microsecond of the first compression and the initial microsecond of the second compression, respectively, during which the plasma undergoes adiabatic compression and heating. The uncertainty in electron-density measurement is ∼10%, introduced by the theoretical uncertainty and the error of the FWHM measurements.45 Electron temperature was measured using line-to-continuum thermometry,47 the theoretical uncertainty of which is negligible, and the accuracy in temperature measurement is better than 10%.
    (a) Detailed evolution of the trapped magnetic field and its derivative, as well as the driving magnetic field, during magnetized plasma compression. (b) Illustrations of magnetic transport in the first compression phase. In each illustration, the outermost ring represents the drive coil, with the driving current flowing counterclockwise. Adjacent to the coil is the vessel wall. Further inside, the ring composed of red and blue curved arrows represents the current sheet, with directional arrows indicating different induced electric fields: the electric field Eθd induced by changes in the driving magnetic field Bd, and the motional electric field Ev×B induced by the bulk plasma motion across the field lines. The blue–gray ringed region displays plasma that has undergone compression, while the uncompressed ambient plasma is situated in front of it. The dot and cross symbols in the diagram represent magnetic fields pointing outward and inward from the page, respectively.
    Plots of Tf/Ti vs nf/ni for adiabatic compression. The adiabatic compression curve is plotted in accordance with the adiabatic relation. The blue star and green square represent the experimental results, corresponding to Stage-1 and Stage-2, respectively.
    Self-luminosity profile of the plasma within the time range under study (taken from Fig. 2), and the associated rates of radiative recombination and three-body recombination.
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    Zhao Wang, Rui Cheng, Xuejian Jin, Yanhong Chen, Lulin Shi, Guodong Wang, Zexian Zhou, Zakir Iqbal, Yupeng Chen, Jinfu Zhang, Xiaoxia Wu, Yu Lei, Yuyu Wang, Yongtao Zhao, Shuai Liu, Liangwen Chen, Jie Yang. Magnetic transport and radiation properties during compression of a magnetized plasma[J]. Matter and Radiation at Extremes, 2025, 10(3): 037401

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    Paper Information

    Received: Oct. 22, 2024

    Accepted: Feb. 13, 2025

    Published Online: Jul. 16, 2025

    The Author Email:

    DOI:10.1063/5.0244786

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