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本文叙述用一维非平衡辐射流体力学激光打靶程序模拟计算高功率密度(~1013W/cm2)激光照射中Z介质薄靶形成的等离子体状态。考虑的物理过程有轫致、光电离、电子碰撞电离及它们的逆过程,Compton散射过程等。Compton散射采用Fokker-Planck近似;电子和离子热传导采用限流扩散近拟;光子方程采用多群限流扩散近似;用平均原子模型计算布居数。激光的吸收主要考虑逆轫致吸收。用功率密度分别为5×1013W/cm2和1×1014W/cm2,波长0.53μm,脉宽450ps的激光从两面和单面打se薄靶,模拟计算结果与国外的实验结果[1]一致。 相似文献
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We have developed and successfully demonstrated the "point projection absorption spectroscopy (hereafter abbreviated to PPAS)" technique to record keV X-ray absorption spectra in the coronal region of laser produced aluminum plasma which provides spatial information in the corona. Absorption spectrum of the Al Ⅻ 1s2-1s2p resonant line for time delays up to 250, 500 and 750 ps after the peak of the incident laser pulse have been observed. Analysis of an absorption spectrum should allow a high spatial resolution (< 25μm) history of the absorbing ion population density to be determined. The 1-D hydro-code JB19 has been used to simulate the experiment and the predictions are compared to the observations. Such comparison can be useful in validating parts of the codes used for gain prediction on recombination X-ray laser transitions. 相似文献
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本文采用新颖的“双靶对接”技术,利用强度~1.2×1013W/cm2,波长1.053μm,脉宽~1ns的两路激光线聚焦辐照平面厚锗双靶,观察到波长为19.6,23.2,23.6,24.7和28.6nm的5根类Ne锗3p-3s跃迁谱线的放大。波长为23.2和23.6nm的谱线,增益长度积GL的值均超过13。对X光激光发射的发散角、折射角及时间特性等,也进行了实验现察,为深入了解X光激光的产生和传播,提供了有意义的信息。 相似文献
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