首页> 外文会议>Conference on Laser-Generated, Synchrotron, and Other Laboratory X-Ray and EUV Sources, Optics, and Applications >Hard X-Ray Spectra from Laser-Generated Plasmas Recorded by the HENEX Spectrometer in the 1 keV - 40 keV Energy Range
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Hard X-Ray Spectra from Laser-Generated Plasmas Recorded by the HENEX Spectrometer in the 1 keV - 40 keV Energy Range

机译:来自Henex光谱仪中的激光产生的等离子体的硬X射线光谱在1 keV - 40 Kev能量范围内记录

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Hard x-ray spectra were recorded by the High Energy Electronic X-Ray (HENEX) spectrometer from a variety of targets irradiated by the Omega laser at the Laboratory for Laser Energetics. The HENEX spectrometer utilizes four reflection crystals covering the 1 keV to 20 keV energy range and one quartz(10-11) transmission crystal (Laue geometry) covering the 11 keV to 40 keV range. The time-integrated spectral images were recorded on five CMOS x-ray detectors. Spectra were recorded from gold and other metal targets and from krypton-filled gasbags and hohlraums. In the spectra from the krypton-filled targets, the helium-like K-shell transitions n = 1-2, 1-3, and 1-4 appeared in the 13 keV to 17 keV energy range. A number of additional spectral features were observed at energies lower than the helium-like n = 1-3 and n = 1-4 transitions. Based on computational simulations of the spectra using the FLYCHK/FLYSPEC codes, which included opacity effects, these additional features are identified to be inner-shell transitions from the Li-like through N-like krypton charge states. The comparisons of the calculated and observed spectra indicate that these transitions are characteristic of the plasma conditions immediately after the laser pulse when the krypton density is 2 x 10~(18) cm~(-3) and the electron temperature is in the range 2.8 keV to 3.2 keV. These spectral features represent a new diagnostic for determining the charge state distribution, the density and electron temperature, and the plasma opacity. The intense 13 keV krypton K-shell emission should be useful for backlighters and radiography of dense plasmas. Laboratory experiments indicate that it is feasible to record K-shell spectra from gold and higher Z targets in the > 60 keV energy range using a Ge(220) transmission crystal.
机译:高能电子X射线(HENEX)光谱记录硬X射线光谱从由OMEGA激光器照射的各种目标进行激光能量学实验室。 HENEX光谱仪利用覆盖1kEV至20keV能量范围的四个反射晶体,覆盖11keV至40keV范围的一个石英(10-11)传输晶体(Laue几何)。将时间集成的光谱图像记录在五个CMOS X射线探测器上。光谱从金和其他金属靶标记录,填充氪气的气囊和HOHLRAUM。在填充氪的靶标的光谱中,氦样K-壳过渡N = 1-2,1-3和1-4出现在13keV至17keV能量范围内。在低于氦样n = 1-3和n = 1-4转变的能量下观察到许多额外的光谱特征。基于使用包括透明度效应的飞奇克/飞行码的光谱的计算模拟,这些附加特征被识别为来自Li的内壳转换通过N样Krypton充电状态。计算和观测的光谱的比较表明,当氪密度为2×10〜(18)cm〜(3)时,这些转变是在激光脉冲之后立即在激光脉冲之后的等离子体条件的特征。 kev到3.2 kev。这些光谱特征表示用于确定电荷状态分布,密度和电子温度和等离子体不透明度的新诊断。强烈的13 kev krypton k-shell排放应该是对致密等离子体的背光和射线照相。实验室实验表明,使用GE(220)传输晶体在> 60keV能量范围内从金和Z靶标记k-shell光谱是可行的。

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