基于固相抗体模式时间分辨荧光免疫分析测定雌三醇

采用二步标记法,借助二乙烯三胺五乙酸酐,将Eu3+标记到雌三醇完全抗原上,基于固相抗体竞争反应模式,建立了时间分辨荧光免疫分析测定雌三醇的新方法。在优化的条件下,方法的线性范围为0.005—1000ng·mL-1,检出限为4pg·mL-1。该方法用于检测血清中雌三醇的含量,结果令人满意。     

Interest-Driven Model for Human Dynamics

Empirical observations indicate that the interevent time distribution of human actions exhibits heavy-tailed features. The queuing model based on task priorities is to some extent successful in explaining the origin of such heavy tails, however, it cannot explain all the temporal statistics of human behavior especially for the daily entertainments. We propose an interest-driven model, which can reproduce the power-law distribution of interevent time. The exponent can be analytically obtained and is in good accordance with the simulations. This model well explains the observed relationship between activities and power-law exponents, as reported recently for web-based behavior and the instant message communications.     

飞秒激光烧蚀铝靶产生喷射物的超快脉冲数字全息诊断

采用脉冲数字显微全息技术,对50 fs单脉冲激光烧蚀铝靶过程中的物质喷射以及等离子体演化的动态过程进行了实验研究,获得了高时空分辨的动态数字全息图.由全息图观察到了热弹力波引起的二次喷射现象,并且报道了大延迟下喷射物质对400 nm探测光所引起的干涉条纹的反常移动现象.通过对全息图进行数字再现,得到了不同延迟下探测光穿过等离子体后的二维相位分布,并运用逆Abel变换算法获得了等离子体折射率以及等效电子密度的时空演化动态过程.根据实验以及计算所得到的有关于喷射物的光学性质,对喷射物的结构和成分进行了分析. 关键词： 脉冲数字全息 飞秒激光烧蚀 超快时间分辨 等离子体     

低强度飞秒激光激发下CdTe和CdTe/CdS核壳量子点的荧光上转换研究

利用400 nm和800 nm不同波长的低强度飞秒激光,对CdTe和CdTe/CdS核壳量子点溶胶进行激发,研究其稳态和时间分辨荧光性质.800 nm飞秒激光激发下,CdTe和CdTe/CdS核壳量子点产生上转换发光现象,上转换荧光峰与400 nm激发下的荧光峰相比蓝移最多达15 nm,而且蓝移值与荧光量子产率有关.变功率激发确认激发光功率与上转换荧光强度间满足二次方关系,时间分辨荧光的研究表明荧光动力学曲线服从双e指数衰减.提出表面态辅助的双光子吸收模型是低激发强度上转换发光的主要机理.CdTe和CdT 关键词： CdTe量子点 CdTe/CdS核壳量子点 时间分辨荧光 上转换荧光     

我国卫星双向时间频率比对结果用于国际原子时归算

国际权度局（BIPM）在最新一期T公报上正式刊登了中国科学院国家授时中心（NTSC）的卫星双向时间频率传递系统结果．至此,中国科学院国家授时中心卫星双向比对结果被正式用于国际原子时归算,中国科学院国家授时中心与国际标准时间UTC比对的A类不确定度也由1．5ns提高到0．5ns,1ns=10^-9s．     

脉冲激光偏振特性用于目标的探测识别

针对光电探测时仅用强度来处理信息的局限性,通过理论分析,提出一种利用脉冲激光反射、散射偏振态时间、空间相关检测的方法,可以克服由于强度差过小带来的目标检测上的困难.利用分析结论,通过计算偏振分布密度函数(Stokes矢量的概率密度函数),进一步讨论了偏振传递函数的特性,用于识别目标,并给出了计算实例.     

激光拉曼光谱实验最优实验参数的确定

讨论了激光拉曼实验中狭缝宽度、阈值大小、积分时间和负高压对拉曼光谱的影响,确定了激光拉曼光谱实验的最佳工作参量,获得了清晰的拉曼光谱.     

Optimization of Pulse Temporal Contrast in Optical Parametric Chirped Pulse Amplification

In optical parametric chirped pulse amplification （OPCPA）, the degradation of temporal contrast of the compressed signal pulse mainly results from spectral clipping in the grating stretcher with finite size of the optics, parametric fluorescence （PF） and the spectral variations transferred from temporal fluctuation of the pump pulse. The temporal contrast of the recompressed amplified pulse in the OPCPA system is studied numerically and a number of solutions are considered and optimized to achieve the highest temporal contrast.     

Lattice Boltzmann Simulations of Particle-Particle Interaction in Steady Poiseuille Flow

The moving behaviour of two- and three-particles in a pressure-driven flow is studied by the lattice Boltzmann simulation in two dimensions. The time-dependent values, including particles＇ radial positions, translational velocities, angular velocities, and the x-directional distance between the particles are analysed extensively. The effect of flow Reynolds number on particle motion is also investigated numerically. The simulation results show that the leading particle equilibrium position is closer to the channel centre while the trailing particle equilibrium position is closer to the channel wall. If Reynolds number Re is less than 85.30, the larger flow Reynolds number results in the smaller x-directional equilibrium distance, otherwise the x-directional distance increases almost linearly with the increase of time and the particles separate finally. The simulation results are helpful to understand the particle-particle interaction in suspensions with swarms of particles.     

Dynamic Processes of Cross-Tail Current in the Near-Earth Magnetotail

Current dynamic processes in realistic magnetotail geometry simulations under various driven conditions and Hall effects. are studied by Hall magnetohydrodynamic （MHD） Associated with the external driving force, a thin current sheet with a broad extent is built up in the near-Earth magnetotail. The time evolution for the formation of the current sheet comprises two phases： slow growth and a fast impulsive phase before the near-Earth disruption of the current sheet resulting from the fast magnetic reconnection. The simulation results indicate that as the external driving force increases, the site and the tailward speed of the near-Earth current disruption region are closer to the Earth and faster, respectively. Whether the near-Earth disruption of the current sheet takes place or not is mainly controlled by Hall effects. It is found that there is no sudden disruption of the current sheet in the near-Earth region if the ion inertial length is below di= 0.04.