首页> 外文会议>Laser-Generated, Synchrotron, and Other Laboratory X-Ray and EUV Sources, Optics, and Applications II >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:HENEX光谱仪记录的激光产生等离子体的硬X射线光谱在1 keV-40 keV能量范围内

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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:硬X射线光谱是由高能电子X射线(HENEX)光谱仪从Omega激光在激光能量学实验室照射的各种目标记录下来的。 HENEX光谱仪使用四个反射晶体,覆盖1 keV至20 keV的能量范围,以及一个石英(10-11)透射晶体(劳厄几何形状),覆盖11 keV至40 keV的能量范围。将时间积分光谱图像记录在五个CMOS X射线探测器上。记录了金和其他金属靶以及gas填充气袋和大喇叭的光谱。在来自targets填充靶的光谱中,类似氦的K壳跃迁n = 1-2、1-3和1-4出现在13 keV至17 keV的能量范围内。在比类氦气的n = 1-3和n = 1-4跃迁低的能量处观察到许多其他光谱特征。基于使用FLYCHK / FLYSPEC代码对光谱进行的计算模拟(其中包括不透明效果),这些附加特征被确定为从Li型到N型k电荷态的内壳转变。计算和观察到的光谱的比较表明,当the密度为2 x 10〜(18)cm〜(-3)且电子温度在2.8范围内时,这些跃迁是紧接在激光脉冲之后的等离子体条件的特征。 keV至3.2 keV。这些光谱特征代表了一种新的诊断方法,用于确定电荷状态分布,密度和电子温度以及等离子体的不透明度。强烈的13 keV K K壳发射应可用于背光源和密集等离子体的射线照相。实验室实验表明,使用Ge(220)传输晶体记录金和更高的Z目标在> 60 keV能量范围内的K壳光谱是可行的。

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