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首页> 外文期刊>Journal of Quantitative Spectroscopy & Radiative Transfer >K-SHELL SPECTROSCOPY OF RADIATIVELY HEATED ALUMINIUM
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K-SHELL SPECTROSCOPY OF RADIATIVELY HEATED ALUMINIUM

机译:辐射加热铝的K壳光谱

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Thin solid tamped foils were heated by the x-rays generated in spherical gold hohlraums which were irradiated by the high power laser ASTERIX IV with an energy of up to 500 J and a pulse duration of 0.4 ns. The sample foils were probed by the radiation of a back-lighter with a variable delay to the main beam. Previous opacity studies in the extreme uv range (G. Winhart et al., PRE, 53, R1332, 1996) have now been completed by measurements in the keV range by using a crystal spectrometer. We present K-shell absorption spectra of aluminium at temperatures between 20 and 30 eV. For the analysis we used local thermodynamic equilibrium opacity codes. The resulting mean ionization of the sample is compared with hydro-code simulations which were post-processed by solving the rate equations using a collisional radiative model.
机译:球形固体金箔中产生的X射线加热了实心夯实的薄箔,然后用高功率激光ASTERIX IV照射,能量高达500 J,脉冲持续时间为0.4 ns。样品箔片通过背光灯的辐射探测,光束延迟到主光束。以前在极端uv范围内的不透明性研究(G. Winhart等,PRE,53,R1332,1996)已经通过使用晶体光谱仪在keV范围内进行测量而完成。我们提出了铝在20至30 eV之间的K壳吸收光谱。为了进行分析,我们使用了局部热力学平衡不透明度代码。将所得样品的平均电离与水码模拟进行比较,后者通过使用碰撞辐射模型求解速率方程来进行后处理。

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