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X-ray absorption spectroscopy for wire-array Z-pinches at the non-radiative stage

机译:非辐射阶段线阵列Z夹的X射线吸收光谱

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Absorption spectroscopy was applied to wire-array Z-pinches on the 1?MA pulsed-power Zebra generator at the Nevada Terawatt Facility (NTF). The 50?TW Leopard laser was coupled with the Zebra generator for X-ray backlighting of wire arrays at the ablation stage. Broadband X-ray emission from a laser-produced Sm plasma was used to backlight Al star wire arrays in the range of 7-9??. Two time-integrated X-ray conical spectrometers recorded reference and absorption spectra. The spectrometers were shielded from the bright Z-pinch X-ray burst by collimators. The comparison of plasma-transmitted spectra with reference spectra indicates absorption lines in the range of 8.1-8.4??. Analysis of Al K-shell absorption spectra with detailed atomic kinetics models shows a distribution of electron temperature in the range of 10-30?eV that was fitted with an effective two-temperature model. Temperature and density distributions in wire-array plasma were simulated with a three-dimension magneto-hydrodynamic code. Post-processing of this code's output yields synthetic transmission spectrum which is in general agreement with the data.
机译:吸收光谱法应用于在内华达州兆瓦级设施(NTF)的1?MA脉冲功率Zebra发生器上的线阵列Z夹片上。 50?TW豹激光与Zebra发生器耦合,用于在烧蚀阶段对线阵列进行X射线背光照明。来自激光产生的Sm等离子体的宽带X射线发射被用于背光在7-9θ范围内的Al星形线阵列。两个时间积分的X射线锥形光谱仪记录了参考光谱和吸收光谱。准直仪将光谱仪屏蔽在明亮的Z夹X射线爆裂下。等离子体透射光谱与参考光谱的比较表明吸收线在8.1-8.4Ω范围内。使用详细的原子动力学模型对Al K壳吸收光谱进行的分析显示,电子温度分布在10-30?eV的范围内,这与有效的两个温度模型相吻合。使用三维磁流体动力学代码模拟线阵列等离子体中的温度和密度分布。此代码输出的后处理产生合成传输频谱,该频谱通常与数据一致。

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