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介绍旨在抑制BaF2闪烁体慢发光成分,拓展其应用领域的紫外滤光膜系设计和性能测量结果,研究表明,以Al2O3/MgF2/Al/MgF2为基本结构优化设计的紫外滤光膜系对来自BaF2闪烁体不同角度入射的快/慢成分光分别具有高透射和强截止特性.还提供了用纳秒级脉冲辐射源激发"BaF2+紫外滤光膜系+光电闪烁探测器"系统获得的BaF2闪烁体时间响应曲线,并对紫外滤光膜系中子辐照损伤特性进行了研究. 相似文献
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介绍旨在抑制BaF2闪烁体慢发光成分,拓展其应用领域的紫外滤光膜系设计和 性能测量结果,研究表明,以Al2O3/MgF2/Al/MgF2为 基本结构优化设计的紫外滤光膜系对来自BaF2闪烁体不同角度入射的快/慢成分光分别具有高透射和强截止特性.还提供 了用纳秒级脉冲辐射源激发“BaF2+紫外滤光膜系+光电闪烁探测器”系统获得的BaF2闪烁体时间响应曲线,并对紫外滤光膜系中子辐照损伤特性进行了研究.
关键词:
2闪烁体')" href="#">BaF2闪烁体
紫外线
滤光片
时间响应 相似文献
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本文报道了2003年在强光一号装置上进行的钨丝阵列的Z箍缩实验研究的主要结果。为了研究钨丝阵列的内爆过程和x光辐射特性,使用了x光功率谱仪和一维时空分辨x光成像系统等诊断设备。实验中由32根5微米钨丝组成的直径8mm长20mm的优化负载获得了最高能量为36.6kJ的x光产额,一维时空分辨x光成像系统的数据显示x光辐射区域以6.4×106cm/s的速度减小,同时x光峰值时刻出现在等离子体被压缩到近轴区域之前。 相似文献
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X-Ray Radiation Characteristics of Nested-Wire Array Implosion in Sino-Russian Joint Z-pinch Experiments on Angara-5-1 总被引:3,自引:0,他引:3 下载免费PDF全文
徐荣昆李正宏 宁佳敏郭存许泽平 杨建伦李林波夏广新 毕欣生丁宁刘强 顾元朝E.V.Grabovsky G.M.Oleynic S.L.Nedoseev V.V.Alexandrov K.N.Mitrofanov M.V.Zurin G.S.Volkov I.A.Porofeev I.N.Frolov V.P.Smirnov 《中国物理快报》2005,22(2):413-415
We report and discuss the results of x-ray radiation measurements in the Sino-Russian joint Z-Pinch experiments on Angara-5-1 facility with a load current of 2.5-3.6MA. The measurements were conducted by using an x-ray power meter (XRPM) and a time-resolved one-dimensional x-ray imaging system developed in China Academy of Engineering Physics. The experimental results indicate that an x-ray power-platform prior to a main peak and a less intensive sub-peak after the main peak in the waveform exist for the nested-wire array implosions, and the radiation process is relatively faster than that in the case of the single array. Laser shadowgraph of the imploding plasma suggests that the prior power-platform is a result of the collision of the inner-outer plasma layers. The faster radiation process of nested array implosion can be explained by analysing the corresponding result of the time-resolved one-dimensional imaging system, which demonstrates a better axial imploding uniformity and synchronization. In comparison with x-ray diode, the XRPM yields a higher height of x-ray power-platform due to its fiat energy response. The sub-peak after the main peak is proposed to be a result of the later-time additional implosion of plasma. 相似文献
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