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Investigation Of Conditions In Closely Spaced Parallel Exploding Aluminum Wires Using Point Projection X-Ray Absorption Spectroscopy

机译:点投影X射线吸收光谱法研究近距离平行爆炸铝线的条件

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This dissertation presents the results of experiments using point-projection absorption spectroscopy to measure conditions with 20[MICRO SIGN]m spatial and sub-ns temporal resolution in closely spaced parallel and single exploding Al wires. Experiments were conducted on both the 0.5 M A XP and 1 M A COBRA generators at Cornell University. The intense continuum radiation pulse from micron scale Mo wire X-pinches was used to backlight the exploding wire plasmas. A spherically bent quartz crystal spectrometer was used to disperse the x-rays which, in conjunction with the small source size, provides very high spectral resolution ([lamda]/[INCREMENT][lamda] ~ 5000) and is ideal for studying the detailed 1 s [-] 2 p and 1 s [-] 3 p absorption spectra in the plasmas generated by Al wire array z-pinches. Absorption features of ionization stages from Mg-like to He-like Al have been identified in spectral structures surrounding the cold K-edge at 7.95Å (1560eV ). This work represents the first time many of the 1 s [-] 3 p features have been observed and identified. Changes in the spectral structure near the K-edge are correlated with the spatial structure of the dense residual wire core. The transition from cold dense core material to the tenuous coronal plasma is observed directly via the spatially resolved change in absorption near the wire core. In the COBRA experiments a step wedge was used to calibrate the expo- sure level on the film, which enabled us to determine the absolute transmission through the plasma within ±17%. A genetic algorithm was developed to fit synthetic spectra calculated using the collisional-radiative code SCRAM to the experimental spectra. This approach allowed the inferred plasma conditions to vary along the line of sight of the diagnostic. The distributions of density and temperature determined by the genetic algorithm are not unique, but were constrained to satisfy several criteria that ensure they are physically reasonable. In the two-wire experiments the temperature reaches 29 ± 7eV in the plasma accumulating at the center line between the two wires. At the edge of the wire cores, where the density remains high ( 0.027g/cc), the temperature is less than 10eV .
机译:本文介绍了点投影吸收光谱法在间隔很近的平行和单根爆炸铝线中以20 [MICRO SIGN] m空间和亚ns时间分辨率测量条件的实验结果。康奈尔大学的0.5 M A XP和1 M A COBRA发生器均进行了实验。来自微米级Mo线X夹的强烈连续辐射脉冲用于照亮爆炸线等离子体。使用球形弯曲石英晶体光谱仪来分散x射线,并结合较小的光源尺寸,可提供非常高的光谱分辨率(λ/ [INCREMENT]λ〜5000),非常适合研究详细的Al线阵列z收缩产生的等离子体中1 s [-] 2 p和1 s [-] 3 p的吸收光谱。已在7.95Å(1560eV)的冷K边缘周围的光谱结构中确定了从Mg样到He样Al的电离阶段的吸收特征。这项工作是第一次观察到并识别出许多1 s [-] 3 p特征。 K边缘附近的光谱结构的变化与致密的残留线芯的空间结构相关。从冷致密芯材料到脆弱的冠状血浆的过渡直接通过线芯附近吸收的空间分辨变化来观察。在COBRA实验中,使用阶梯楔形物校准薄膜上的曝光水平,这使我们能够确定通过等离子体的绝对透射率在±17%以内。开发了一种遗传算法,以将使用碰撞辐射代码SCRAM计算的合成光谱拟合到实验光谱中。这种方法允许推断出的血浆状况沿着诊断的视线变化。遗传算法确定的密度和温度分布不是唯一的,但必须满足几个条件以确保它们在物理上是合理的。在两线实验中,在两线之间的中心线积聚的等离子体中,温度达到29±7eV。在密度较高的线芯边缘(0.027g / cc),温度低于10eV。

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    Knapp Patrick;

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  • 年度 2011
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