轴向拉伸对Ni纳米线结构和稳定性的影响

采用推广模拟退火算法和Sutton Chen势, 选取fcc[111]结构的Ni纳米线为初始构型, 研究了轴向拉伸对Ni纳米线的结构和稳定性的影响。 研究结果表明: 拉伸程度的大小对Ni纳米线的结构和稳定性有很大的影响; 随着拉伸强度的变化, 纳米线结构分别为fcc[111]结构、 (6, 0)型管＋中心柱状结构（又为螺旋结构）、 (6, 3) 型管＋中心柱状结构、 fcc[110]结构、 过渡结构（为规则结构）和缺陷结构; 从结合能分布来看, 结合能先减小, 再增大, 结合能最小时对应最稳定结构 (6, 0) 型管＋中心柱状结构（又为螺旋结构）。 Atomic structures and stabilities of Ni nanowires are studied by using the generalized simulated annealing method with Sutton Chen potential. The initial structure is face centered cubic [111] structure. The result shows that the length of the supercell strongly affects the structures and stabilities of Ni nanowires. fcc [111] structure, (6, 0), (6, 3) nanowires, fcc[110], transition structure and defect structure are found for different wire lengths. And from the analyses of the binding energy, it is found that (6, 0) nanowires (helical structure) is the most stable form.     

Restoration of solar and star images with phase diversity-based blind deconvolution

The images recorded by a ground-based telescope are often degraded by atmospheric turbulence and the aberration of the optical system. Phase diversity-based blind deconvolution is an effective post-processing method that can be used to overcome the turbulence-induced degradation. The method uses an ensemble of short-exposure images obtained imultaneously from multiple cameras to jointly estimate the object and the wavefront distribution on pupil. Based on signal estimation theory and optimization theory, we derive the cost function and solve the large-scale optimization problem using a limited memory Broyden-Fletcher-Goldfarb-Shanno (L-BFGS) method. We apply the method to the urbulence degraded images generated with computer, the solar images acquired with the swedish vacuum solar telescope (SVST, 0.475m) in La Paima and the star images collected with 1.2-m telescope in Yunnan Observatory. In order to avoid edge effect in the restoration of the solar images, a modified Hanning apodized window is adopted.The star image till can be estored when the defocus distance is measured inaccurately. The restored results demonstrate that the method is efficient for removing the effect of turbulence and reconstructing the point-like or extended objects.     

钢铁检测微型光谱仪的研制

针对国内光电直读型钢铁检测微型光谱仪研究的不足,提出基于Czerny-Turner结构的系统设计方法,讨论了优化方法及验证方法,并加工出了光谱仪。光谱仪采用三次多项式拟合标定波长,实测分辨率在436 nm~608 nm全谱段达0.225 nm、中心谱段达0.135 nm,基本满足钢铁检测要求。提出一种基于多帧判断的定性分析方法,7种待测元素检出限优于1.5%,通过建立拟合光谱数据库实现半定量分析,25种样品检测精度达2%,为钢铁牌号识别提供重要参考。     

中和颗粒可压缩性颗粒层模型

本文针对可压缩颗粒层建立了二维数值模型.首先利用颗粒层中颗粒间的相互位置关系,建立了每一个颗粒的力平衡方程,获得了每一个颗粒的受力大小,然后提出了颗粒层坍塌判据,在此基础上,建立了描述颗粒层的沉积-压缩-沉积的动态过程的可压缩颗粒层模型,模型计算结果表明,颗粒层压缩现象主要发生在下部区域,过滤速度越高、范德华力越小,颗粒层越易坍塌,并且颗粒层的压降出现了脉动,模型结果符合已知的实验结果.     

Vector meson rescattering effect in understanding the threshold enhancement observed in J/ψ→γp(p)

We propose one possible mechanism,i.e.,the vector meson(VV)rescattering effects,to interpret the near threshold narrow enhancement observed in J/ψ→γp(p).The estimate indicates that these effects can give sizeable contributions to this channel,and a destructive interference between different rescattering amplitudes is required to reproduce the line shape of the data.     

300～1100nm多波段成像光学系统设计及杂光分析

设计了一套300～1100nm多波段光学系统,该系统能对目标的近紫外、可见光和近红外3个波段同时成像,可满足目标多波段信息探测的要求。由于在光学系统中镜筒内壁反射和棱镜表面反射会产生杂光和鬼像,因此,利用Light—Tools软件对此系统的杂光和鬼像进行了模拟分析。模拟结果表明,视场之外11．7—18．3°和-11．7～-18．3°的入射光线被胶合棱镜上下表面反射后,会聚焦到3个探测器靶面范围内,形成鬼像;6．2°-9．8°和一6．2°--9．8°的入射光线被镜筒反射后会在3个探测器上形成杂光。利用设计的多波段光学系统进行了相关实验,结果证明了模拟分析的正确性,表明此分析能用于指导多波段光学系统的设计和研制。提出了减少杂光和鬼像的相应措施,实验结果验证了提出的措施能够减少杂光及消除鬼像,提高系统成像质量。     

传质特性对光纤生物制氢反应器性能的影响

光生物制氢反应器的传质特性是影响反应器特性的重要因素.本文通过构造新型的光纤生物制氢反应器,采用生物膜法细胞固定化技术,考察在连续产氢条件下,进口底物浓度和流速对与反应器产氢相关特性的影响.结果表明:高浓度下出现的底物抑制现象是限制反应器性能的原因;流速改变的传质特性对反应器性能的影响,反映在驱动势和反应时间两个方面.     

激光击穿光谱技术监测固土过程中阳离子交换

为了实时探测离子土固化剂(ISS)在固土过程中的阳离子交换量(CEC),采用激光击穿光谱技术(LIBS),对ISS处理后的土壤溶液中的K、Ca、Na、Mg、Al、Si这6种离子含量进行探测。分别对由不同配比(1∶100、1∶200和1∶300)的ISS处理过的高岭土、膨胀土、红粘土等5种标准土壤进行了研究,结果表明:同一土壤中的各种离子随ISS配比的变化趋势各不相同;不同土壤与ISS作用的效果各不相同;ISS的配比并非越高越好。这些工作为ISS固化机理的研究提供实验依据,而利用激光击穿光谱技术进行探测的方式为ISS固化机理的研究提供了新的思路。     

Irradiation Test of FPGA for BES-Ⅲ

The irradiation effect of FPGA, applied in Front-end Electronics for experiments of High-Energy Physics, is a serious problem. The performance of FPGA, used in the front-end card of Muon Counters of BES-III project, needs to be evaluated under irradiation. SEUs on Altera ACEX 1K FPGA, observed in the experiment under the irradiation of γ ray, 14 and 2.5MeV neutrons, was investigated. We calculated involved cross-section and provided reasonable analysis and evaluation for the result of the experiment. The conclusion about feasibility of applying ACEX 1K FPGA in the front-end card of the readout system of Muon Counters for BES-III was given.