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Measurement of Radiative Collapse in 2.2 kJ PF: Achieving High Energy Density (HED) Conditions in a Small Plasma Focus

机译:在2.2 kJ PF下测量辐射塌陷:在小等离子体焦点下实现高能量密度(HED)条件

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摘要

Radiative collapse in the plasma focus (PF) pinch creates extreme high energy density (HED) in the laboratory. The Pease-Braginskii current is that current flowing in a hydrogen pinch which is just large enough for bremsstrahlung to balance Joule heating; this threshold value being 1.4 MA. For high-Z gases undergoing strong line-radiation the radiation-cooled threshold current is considerably lowered. Recent work applied to a MJ PF has revealed that even if a threshold current is exceeded there is a condition that the characteristic depletion time of the pinch energy by radiation should be of the order of the pinch time in order for strong radiative collapse to be observed, thus explaining why no radiative collapse may be expected in deuterium; and also in helium; even in multi-MA PF devices. This paper extends the computation of depletion times to a kJ PF, the INTI PF showing that in the INTI PF only a small reduction in radius ratio may be anticipated in Ne whilst in Ar, Kr and Xe strong radiative collapse is expected. Two useful Tables are obtained applicable to kJ PF devices, one of reduced Pease-Braginskii currents in various high-Z gases and the other of corresponding characteristic depletion times. Two earlier papers using the Lee code had already demonstrated that radiative collapse occurs in plasma focus operated in high-Z gases. However in those papers computation could only be carried out up to a cut-off radius set at 0.01 of anode radius. Thus as shown in this paper most of the radiative compression was not computed or measured. This paper reports the measurement of the pinch trajectory in Kr by the fitting of a measured current waveform using the code with the cut-off radius successfully removed, so that the fitting fully follows the compression to its minimum radius and beyond to the rebound of the trajectory. The measured current waveform shows radiative collapse to a minimum radius ratio of 0.0014 or 0.0013 cm. Ion density reached 3.7 x 10(26) m(-3); and an immense burst of radiation is emitted with peak power of 10(12) W, radiating 30 J in 50 ps, during the time of peak radiative compression. The energy density at peak compression is 4 x 10(13) J m(-3) or 40 kJ mm(-3). This is the first time such a measurement has been made; and indicates that even in a kJ plasma focus, such a HED state is achieved.
机译:等离子体聚焦(PF)夹点中的辐射塌陷会在实验室中产生极高的能量密度(HED)。 Pease-Braginskii电流是在氢夹流中流动的电流,该夹流的大小足以使致辐射体平衡焦耳热。该阈值为1.4 MA。对于经受强线辐射的高Z气体,大大降低了辐射冷却的阈值电流。应用于MJ PF的最新工作表明,即使超过阈值电流,也存在这样一种条件,即由于辐射而产生的收缩能量的特征耗尽时间应为收缩时间的量级,以便观察到强烈的辐射塌陷。 ,从而解释了为什么在氘中不会发生辐射塌陷;还有氦气即使在多MA PF设备中。本文将耗尽时间的计算扩展到了kJ PF,INTI PF表明,在INTI PF中,预计Ne中的半径比只有很小的减小,而在Ar,Kr和Xe中则有望出现强烈的辐射塌陷。获得了适用于kJ PF器件的两个有用表,一个是在各种高Z气体中降低的Pease-Braginskii电流,另一个是相应的特征耗尽时间。先前使用Lee代码的两篇论文已经证明,在高Z气体中操作的等离子体聚焦中会发生辐射塌陷。但是,在那些论文中,只能进行最大截止半径设置为阳极半径0.01的计算。因此,如本文所示,大多数辐射压缩未得到计算或测量。本文报告了通过使用已成功去除截止半径的代码拟合测量到的电流波形来测量以Kr为单位的收缩轨迹的过程,从而使拟合完全遵循压缩到其最小半径并超出了回弹的回弹的情况。弹道。测得的电流波形显示辐射塌陷至最小半径比为0.0014或0.0013 cm。离子密度达到3.7 x 10(26)m(-3);在峰值辐射压缩期间,以10(12)W的峰值功率发射出大量辐射,以50 ps辐射30J。峰值压缩时的能量密度为4 x 10(13)J m(-3)或40 kJ mm(-3)。这是第一次进行这种测量。并且表明即使在kJ等离子体聚焦下,也达到了这种HED状态。

著录项

  • 来源
    《Journal of Fusion Energy》 |2016年第4期|702-708|共7页
  • 作者

    Saw S. H.; Lee S.;

  • 作者单位

    Nilai Univ, 1 Persiaran Univ, Nilai 71800, Negeri Sembilan, Malaysia|Inst Plasma Focus Studies, 32 Oakpk Dr, Chadstone, Vic 3148, Australia;

    Inst Plasma Focus Studies, 32 Oakpk Dr, Chadstone, Vic 3148, Australia|Univ Malaya, Kuala Lumpur, Malaysia|INTI Int Univ, Nilai 71800, Malaysia;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Plasma focus numerical experiments; Radiation cooling; Radiation collapse; Plasma focus radiation enhancement; Plasma focus HED;

    机译:等离子体聚焦数值实验;辐射冷却;辐射塌陷;等离子体聚焦辐射增强;等离子体聚焦HED;
  • 入库时间 2022-08-18 00:40:15

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