工艺参数对铀表面铝镀层热应力分布影响

为了防止铀的腐蚀，采用在铀表面磁控溅射镀铝，但使用中发现铝镀层内产生了较大的应力，影响镀层结合强度及使用性能。通常认为，薄膜内的应力有热应力和生长应力两种。文中通过改变沉积温度、镀层厚度以及镀层力学性能分数，研究它们对镀层热应力分布的影响，从而为改善铀表面铝镀层内热应力分布提供理论依据。     

浅析XRN技术及其在校园网中的应用

文章介绍了XRN技术的基本概念、原理及主要优势,并探讨了XRN技术在校园网中的应用,同时也提出了一些相应的解决方案。     

回归模型中异方差或变离差检验问题综述

回归模型的异方差或变离差检验是统计诊断的重要课题。本文系统介绍了普通回归模型、广义回归模型和基于纵向数据的随机效应或自相关回归模型的异方差检验或变离差检验的研究概况和最新进展；同时介绍了作者关于非线性回归模型的相应工作，最后指出了若干有有待进一步研究的问题。     

A non-commutative time-frequency tomography

The characterization of non-stationary signal requires joint time and frequency information. However, time and frequency are a pair of non-commuting variables that cannot constitute a joint probability density in the time-frequency plane. The time-frequency distributions have difficult interpretation problems arising from negative and complex values or spurious components. In this paper, we get time-frequency information from the marginal distributions in rotated directions in the time-frequency plane. The rigorous probability interpretation of the marginal distributions is without any ambiguities. This time-frequency transformation is similar to the computerized axial tomography (CT or CAT) and is applied to signal analysis and signal detection and reveals a lot of advantages especially in the signal detection of the low signal/noise (S/N).     

年龄相关的种群扩散系统的最优分布控制

本文讨论年龄相关的种群扩散系统的最优分布控制 ,证明了最优分布控制的存在性 ,得到了分布控制为最优的充分必要条件及确定最优控制的最优性组 .     

面阵探测器的像点亚像素定位研究

面阵探测器可直接探测点目标图像的位置，但其定位精度受到探测器分辨率的限制。因此，亚像元精度技术得到了发展。它是利用目标像点的灰度分布特性，通过内插细分算法，确定出像点位置。可将定位精度提高1—2个数量级。本文介绍了几种实现目标像点亚像素定位的内插细分算法。对它们的计算公式、特点进行了分析，并进行了实验验证。     

Electrical Resistance Measurement of an Individual Carbon Nanotube

Aiming at the difficulty in the electrical resistance measurement, we develop a simple statistical model for the carbon nanotubes adequately dispersed in available insulated liquid and introduce the concept of “the most probability”. Based on this model, we obtain the function between macroscopic resistance R and resistance of an individual nanotube, Ro, from which one can calculate the resistance of an individual nanotube by measuring the macroscopic resistance. By computational simulation, we prove the reliability of the model. Then, we analyse the feasibility of the model when applied to experiment.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．