共查询到20条相似文献,搜索用时 125 毫秒
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传统的塑料闪烁体由于其低有效原子序数和密度,不适用于能谱探测领域。有机重金属化合物掺杂塑料闪烁体的制备为塑料闪烁体实现能谱探测提供了一种有效途径。而有机锡化合物掺杂塑料闪烁体具有高光峰灵敏度,并保留了塑料闪烁体的快衰减特性。本文通过自由基聚合的方法成功制备了不同浓度2-(三丁基锡烷基)呋喃掺杂的聚乙烯基甲苯(PVT)基塑料闪烁体,并对其光学和闪烁性能进行了测试和比较。其中掺杂20%2-(三丁基锡烷基)呋喃的PVT基塑料闪烁体的透光率可达90%,X射线激发发射光谱主峰位于425 nm处,光产额为6700 ph/MeV,能量分辨率为15.8%@662 keV,衰减时间约为4.3 ns。我们也制备了1英寸直径、掺杂20%2-(三丁基锡烷基)呋喃的塑料闪烁体,具有6300 ph/MeV的光产额和15.8%@662 keV的能量分辨率。 相似文献
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具有许多优点的塑料闪烁体广泛应用在粒子物理中. 高能高电荷情形下塑料闪烁体的光响应研究在高能物理和宇宙线物理中有着重要意义. 芝加哥大学的高能宇宙线实验, 除了获得许多重要天体物理结果, 还为塑料闪烁体对高电荷相对论粒子的光响应研究积累了资料. 本文介绍上述宇宙线实验和资料分析结果并对塑料闪烁体的非线性光响应进行讨论. 相似文献
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《物理与工程》2015,(4)
多像素光子计数器(Multi Pixel Photo Counter,简称MPPC)是近几年发展起来的一种新型信号读出设备.为了对这种设备制作的闪烁探测器有较深入的了解和认知,本文配合塑料闪烁体,与MPPC制成塑料闪烁探测器,对利用这种新型的光子计数器做成的探测器进行了研究.利用它测试了塑料闪烁体的时间和位置分辨率,将这方面数据与之前常用的配有光电倍增管的闪烁探测器的数据进行了比较,能够了解到用MPPC与塑料闪烁体做成的闪烁探测器在时间分辨和位置分辨方面能够达到实验的要求.在信价比和几何大小方面,MPPC优于光电倍增管,因此利用MPPC将在实验方面带来很大的优越性,为实验研究提供更大的方便. 相似文献
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L. G. Efimov E. M. Kislov N. S. Moroz Yu. A. Panebrattsev V. I. Yurevich A. N. Zubarev 《Physics of Particles and Nuclei Letters》2009,6(3):236-240
Two special experimental facilities have been designed and produced to provide charged particle tests of the Transition Radiation
Detector (TRD) prototypes and modules for the ALICE experiment at CERN. The first facility, comprising the scintillation and
Cherenkov detectors, was applied for the TRD elements investigation with a secondary mixed electron-pion beam of the CERN
proton synchrotron PS. The second one, consisting of two large-scale scintillation planes and original electronics, is under
operation to trigger the 7-m long TRD supermodules on closing stand-alone trial with cosmic particles. The design and performance
of both facilities are considered.
The article is published in the original. 相似文献
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Kiyohide Miyake 《Optical and Quantum Electronics》1981,13(1):1-10
The effect of atmospheric turbulence on the accuracy of optical pulsed range measurements is investigated assuming a Poisson detection process and log normal scintillation. Expressions for the detection cell and the r.m.s. error of detection in the presence of atmospheric scintillation are derived assuming that the optical pulse duration is long compared to the correlation time of the atmospheric scintillation, and evaluated numerically for various optical Gaussian pulse shapes. Numerical results show that in the presence of weak scintillation, the r.m.s. detection error depends primarily on the number of photoelectrons in the pulse, while in the presence of strong scintillation, it depends largely on the strength of scintillation as well as the number of photoelectrons in the pulse. It is also found that the detection error depends largely on the pulse width and the resolution time of the photodetector in the presence of atmospheric scintillation. 相似文献
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为了有效抑制激光大气传输过程中引起的闪烁效应,本文围绕照明光束相干性与闪烁指数关系展开研究。首先,明确闪烁效应产生机理,建立与光束相干性相关的数学模型。然后,采用偏振分光元件将出射激光分为4束,并破坏其相干性。在此基础上,以随机相位屏为核心元件构建大气湍流仿真实验装置,评估不同光束相干性条件下的远场光斑闪烁指数。实验结果表明,4束光照明的光斑闪烁指数比单光束照明降低了75%。理论分析及实验结果均证明了多束部分相干光在抑制光强闪烁效应方面的有效性。 相似文献
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利用中子飞行时间技术和BC501A液体闪烁探测器的粒子分辨特性,测量了0°方向、20 MeV氘束轰击厚金属铍靶反应产生的中子源能谱,测量的中子能谱范围为0.7~25.0 MeV。在60°方向放置芪晶体闪烁探测器,由刻度好的BC501A液体闪烁探测器归一校正后,用于中子源强度监测。利用Be(d, n) 反应中子源,采用单粒子灵敏度标定方法,实验标定了0.75~15.75 MeV能量范围内的薄膜闪烁探测器中子能量响应曲线,实验结果与蒙特卡罗模拟计算结果在8%的不确定度范围内一致。 相似文献
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在远场散斑投影成像系统上整合大气闪烁指数测量功能,有助于全面分析激光大气传输特性及其对光电系统性能的影响。但是在大口径接收时,大气闪烁会因孔径平滑效应而变得微弱,光源稳定性引起的强度起伏会更为明显。针对这一问题,基于光源强度起伏和大气闪烁的乘性调制假设,建立了考虑光源强度起伏的大气闪烁指数的测量模型。利用光源强度起伏不随孔径变化而大气闪烁随孔径变化这一差异性,通过投影光学在同一时刻测量两个不同接收孔径上的光强闪烁,结合弱起伏条件下的孔径平滑因子来求解测量模型,从而分别估计大气闪烁指数和光源强度闪烁指数。实验结果表明,在孔径0.05m至0.4m之间,实测值和理论估计值的最大相对误差小于9.685%,理论模型与实验符合度较高。采用该方法可以在投影光学上实现弱起伏条件下的大气闪烁指数估计。 相似文献
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A. V. Bakaldin S. A. Voronova A. A. Kvashnin A. N. Kvashnin E. F. Maklyaev Yu. S. Maksumov Yu. I. Stozhkov 《Bulletin of the Lebedev Physics Institute》2015,42(12):333-337
An array of scintillation detectors of the MONICA Spectrometer, whis is aimed at investigating fluxes of cosmic-ray ions (from H to Ni) in the extraterrestrial space within the energy range from 10 to 300 MeV per nucleon, is considered. The basic goal of the MONICA experiment is the measurement of the ionic and isotopic composition of cosmic rays of the galactic and solar origin, as well as the measurement of their energy spectrum. This problem was intensely studied by numerous investigators [1–10]; nevertheless, a lot of questions remain unsolved up to now, in this field of science. The array of scintillation detectors plays the important role in achieving the goals of the MONICA experiment. The composition of the array, tuning procedure, and characteristics of scintillation detectors are discussed in detail. 相似文献
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The power spectral density function (PSDF) of the log-amplitude scintillation for an infrared laser beam was measured experimentally. To investigate the contribution of the absorption and the dispersion that cause the scintillation, we chose 16 wavelengths of infrared light and one wavelength of visible light. It is found that the spectral density of scintillation for the infrared beam does not agree with that for the visible beam, as predicted by Tatarskii's theory in the low-frequency region below 1 Hz. This disagreement between the experiment and the theory in the low-frequency region should be attributed to water vapour absorption. 相似文献