散射介质中层间杂质检测效率的影响因素及分析

散射介质中层间杂质检测是一个非常重要的研究课题.改进现有的Monte Carlo方法,模拟大量光子在散射介质中的传输,得到入射光强、杂质埋藏深度、介质折射率、介质散射系数和各向异性因子对光学透反射成像法检测层间杂质效率的影响规律.结果表明,入射光强、杂质埋藏深度和介质折射率对透反射成像检测结果均有影响,且影响规律相似.增加入射光强、减小杂质埋藏深度或减小介质折射率均可提高反射光成像的检测效率;增大入射光强、减小介质折射率、减小介质散射系数或增大各向异性因子均可提高透射光成像的检测效率.这些规律对散射介质中层间杂质检测具有一定指导意义.     

Checking for normality in linear mixed models

Linear mixed models are popularly used to fit continuous longitudinal data,and the random effects are commonly assumed to have normal distribution.However,this assumption needs to be tested so that further analysis can be proceeded well.In this paper,we consider the Baringhaus-Henze-Epps-Pulley (BHEP) tests,which are based on an empirical characteristic function.Differing from their case,we consider the normality checking for the random effects which are unobservable and the test should be based on their predictors.The test is consistent against global alternatives,and is sensitive to the local alternatives converging to the null at a certain rate arbitrarily close to 1/√ n where n is sample size.Furthermore,to overcome the problem that the limiting null distribution of the test is not tractable,we suggest a new method: use a conditional Monte Carlo test (CMCT) to approximate the null distribution,and then to simulate p-values.The test is compared with existing methods,the power is examined,and several examples are applied to illustrate the usefulness of our test in the analysis of longitudinal data.     

非参数空间滞后模型的广义矩估计北大核心CSCD

放松了参数空间滞后模型中自变量的影响为已知的线性或非线性形式假设,考虑一类非内生自变量为随机变量的非参数空间滞后模型,构建了该模型的广义矩估计法,导出了其估计量的渐近性质,用Monte Carlo模拟方法考察了估计量的小样本表现.此外还将所提出的估计方法应用于估算我国各省市全要素生产率增长率.     

生物组织中激光传输规律的模拟与检验

本文研究了激光在生物组织中的传输规律,建立了适用于Monte Carlo模拟的数理模型。对不同组织中光子的传输规律进行了模拟和检验,结果表明:利用本文所建立的模型和编制的程序,可以有效地模拟激光在均匀和非均匀组织中的传输规律,并可获取组织光学特性参数与漫反射率、漫透射率和通量等物理量间的关系。     

Monte Carlo方法计算晶体析出相的X射线发射强度

本文提出了用Monte Carlo模拟计算晶体中析出相X射线发射强度的理论和方法。作为实例,对不同加速电压下Au,Cu基体中Cr—Fe—Ni合金析出相的X射线发射强度作了计算,并得出一些规律。     

Melting properties of mixed Ni13-xAlx(x=0 to 13) clusters

Starting from the configuration full optimized by Genetic Algorithm (GA), the melting behaviors of Binary Ni13-xAlx(x=0 to 13) clusters have been investigated by Monte Carlo (MC) simulations with Metropolis algorithm with a n-body Gupta potential. In contrast to bulk, these clusters have smeared first order transitions occurring over a range of temperature. The melting temperature Tm calculated from Lindemanns criterion vary drastically with concentrations x. For most clusters studied, the average energy per atom E, the relative root-mean-square (rms) bond length fluchuation δ and the heat capacity C per atom related to the energy fluctuation of the system change with temperature in the transition region in manners differing from LJ and alkali metal clusters. For Ni12Al, Ni7Al6, Ni6Al7, Ni5Al8 clusters, there are behaviors characteristic of magic number in C, which do not exist in the pure TM clusters.     

多部雷达最佳部署的遗传算法研究

本文研究了多部雷达联合发现目标概率 ,并采用 Monte Carlo模拟计算面积和遗传算法寻优相结合来计算多部雷达最佳部署 .文中给出了多部雷达部署的一般公式 ,并对雷达数目为 2、3、4的情况进行了计算     

Performance modeling of the adaptive optics system on the 2.16 m telescope

The adaptive optics system on the 2.16 m telescope is modeled and simulated using an ends-to-ends Monte Carlo method in this paper.Under the optimized parameters,the Strehl ratio can be increased from about 0.02 to more than 0.2 in the J,H and K bands with a classical adaptive optics system.Based on the simulation results,the practical system design is also considered and discussed.     

Stochastic Resonance and Ratchets： Two Closely Related Phenomena in Brownian Motors

Ratchet effect as well as the phenomenon of stochastic resonance (SR) is investigated in a simple flashing ratchet model. Numerical simulations show that both the power spectrum amplitude and the mean mobility of the system vary non-monotonically in similar manners with increasing the noise intensity and both reach their highest point nearly at the same noise level. We point out that the consistency of these two phenomena are just due to the existence of circular flux in non-equilibrium state.     

非饱和势模型关于e~＋e~－→qq→h’s的Monte－Carlo模拟

根据非饱和势模型对ｅ＋ｅ－→ｑｑ→ｈ’ｓ过程作了全面的Ｍｏｎｔｅ－Ｃａｒｌｏ模拟．采用一个近似于快度均匀分布的相对纵动量分布，并利用一个与非饱和势模型相一致的方法处理了重粒子衰变．最后把Ｍｏｎｔｅ－Ｃａｒｌｏ模拟结果同２９和３５ＧｅＶ的实验作了比较．