Binary and millisecond radio pulsars

Recent pulsar surveys, especially those using the multibeam receiver on the Parkes radio telescope, have more than doubled the number of known pulsars, bringing the current total to about 1720. Of these, 171 have millisecond periods, 126 are members of binary systems and 99 are associated with globular clusters. Binary pulsars may be divided into several distinct groups depending on their observed properties such as pulsar period and age, binary period, eccentricity and companion mass. These groups all have different evolutionary histories. Correlations between the various properties are discussed using the increased samples now available. The Parkes Pulsar Timing Array is a project which has the goal of using timing observations of millisecond pulsars to make a direct detection of gravitational waves. The parameters and present status of the project are briefly discussed.     

XMM-Newton observations of faint X-ray sources in globular clusters

Using the new generation of X-ray observatories, we are now beginning to identify populations of close binaries in globular clusters, previously elusive in the optical domain because of the high stellar density. These binaries are thought to be, at least in part, responsible for delaying the inevitable core collapse of globular clusters and their identification is therefore essential in understanding the evolution of globular clusters, as well as being valuable in the study of the binaries themselves. Here, we present observations made with XMM-Newton of six globular clusters, in which we have identified neutron star low mass X-ray binaries and their descendants (millisecond pulsars), cataclysmic variables and other types of binaries. We discuss not only the characteristics of these binaries, but also their formation and evolution in globular clusters and their use in tracing the dynamical history of these clusters.     

基于灰色预测的自适应解耦控制

传统的预测控制算法虽然有着良好的性能,但是需要求解复杂的丢番图方程.因而在实际应用中,算法的计算量很大,难以满足实时性要求.文中结合灰色理论,利用GM(1,2)模型辨识多输入多输出系统的参数,提出了一种解耦灰色预测控制算法.该算法可以采用较少的数据进行建模,需要辨识的参数也较少,并且元需求解丢番图方程,所以减少了计算量.为了消除系统各通道之间的输入输出耦合,在性能指标中引入解耦因子,给出了详细的解耦推导过程.最后,对解耦灰色预测控制算法进行了设计.仿真结果表明:本文算法能够有效地消除系统耦合,进而提高多输入多输出系统的闭环跟踪性能.     

复合材料层合板结构的广义强度准则

在试验研究的基础上,将复合材料层舍板看作一个"宏观各向异性板",提出了一种基于试验的复合材料层合板结构广义强度准则的二次完备表达式,并分析了表达式中各参数的试验求解方法.对3种典型铺层的层合板进行纵向拉伸、纵向压缩、横向拉伸、横向压缩、面内剪切等简单裁荷以及双向拉伸、拉剪组合(纵向、横向)等组合栽荷试验.给出了不同铺层形式下广义强度准则表达式中各项系数值.采用该强度准则预测复杂应力状态下的破坏应力与试验值吻合较好.     

含时滞结构线性时变系统伺服机构设计的PGOPO法

采用线性、连续、有界算子－分段广义正交多项式算子对含时滞结构的线性时变系统的线性伺服机构设计问题进行了研究,得到了一种形式简洁、计算精度较Ｗａｌｓｈ函数、块脉冲函数法更高的逼近方法。文中所列举的两个例子充分说明了分段广义正交多项式算子法在时滞系统伺服机构设计中的适用性和有效性。     

灰色关联投影法在近程武器系统综合效能模糊评估中的应用

给出了利用灰色关联投影法解决武器系统多指标综合效能模糊评估问题的基本原理和步骤,并以6种具有典型代表意义的近程武器系统为例,按照给出的步骤,代入数据进行计算,得到的结论验证了方法的正确性和可行性。     

基于PC/104总线的飞机电源产品综合测试系统

详细介绍了一套基于PC／104总线和虚拟仪器技术的飞机电源产品综合测试系统的功能和软硬件实现原理。阐述了测试系统的设计原理，最后结合整个系统设计介绍了在LabVIEW环境下测试系统软件的设计和实现。     

等维灰数递补动态预测在机场客运量预测中的应用

基于灰色系统等维灰数递补动态预测和残差GM（1，1）修正模型，对其应用的可行性进行了有益的探讨，并结合实例，对首都国际机场中短期客运量进行了预测。通过调整原始样本中的变异数据，得到比较理想的预测结果．经检验预测结果是可信的。该研究为机场客运量预测提供了一种方法，可供借鉴。     

双尾撑布局无人机总体气动设计研究进展

介绍了双尾撑布局飞机的起源和特征,讨论了大展弦比和中等展弦比双尾撑布局无人机的设计特点和区别,归纳了双尾撑无人机总体气动设计工具、经验估算公式和阻力特性;指出将统计方法和数值模拟方法相结合,进行多学科设计优化是可行的解决方案,并对未来可能的设计方向进行了展望。     

Observations of Extended Radio Emission in Clusters

We review observations of extended regions of radio emission in clusters; these include diffuse emission in ‘relics’, and the large central regions commonly referred to as ‘halos’. The spectral observations, as well as Faraday rotation measurements of background and cluster radio sources, provide the main evidence for large-scale intracluster magnetic fields and significant densities of relativistic electrons. Implications from these observations on acceleration mechanisms of these electrons are reviewed, including turbulent and shock acceleration, and also the origin of some of the electrons in collisions of relativistic protons by ambient protons in the (thermal) gas. Improved knowledge of non-thermal phenomena in clusters requires more extensive and detailed radio measurements; we briefly review prospects for future observations.