直升机飞行学员培训数学模型与需求预测

通过轻型直升机飞行人员培训的建模环境及目前中国通用航空的现状与国外通用航空的比较,提出了中国发展通用航空需求预测的数字化方法,建立了飞行人员培训的数学模型,做出了飞行人员培训的动态分析,为有计划地培养直升机飞行人员提供可靠依据。所推导出的数学模型也适用于运输机飞行员培训预测并为提高运输机飞行员培养教育开辟一个新途经。     

基于最小二乘法的分解炉温度控制数学模型

根据分解炉温度控制的实际生产情况,确定了三次风、煤粉和生料流量与分解炉温度之间的关系,建立了分解炉温度控制的数学模型。由于神经网络可以实现对复杂非线性对象进行卓有成效的控制,因此选定神经网络中应用最广泛的BP神经网络作为控制算法,对三次风和煤粉阀门开度进行控制,从而实现对分解炉温度预测控制。     

水下爆轰燃气泡形态与激波传播过程研究*(爆震专刊)

针对脉冲爆轰发动机在水下工作过程中形成的燃气射流问题,搭建了水下爆轰燃气实验系统,研究了第一个爆轰循环在水下的燃气泡发展变化过程。建立了基于气液两相双流体模型的脉冲爆轰发动机水下喷射模型,采用时-空守恒元和求解元方法,模拟了爆轰波退化为激波在水中的传播及衰减过程。研究结果表明：燃气泡前期受外界水环境阻滞作用呈现“豌豆状”形态,充分发展阶段气液交界面逐渐失稳,在达到最大尺寸后开始收缩并在中心轴线位置出现凸出的射流；水下爆轰燃气射流发展过程中同时存在脱离燃气泡的水中前导激波和管口燃气泡内的高压区两部分,水中前导激波在传播过程中压力迅速衰减至常压量级,而管口燃气泡内则一直保持较高压力；中心轴线区域气液交界面处反射激波的回传使管口附近出现回击现象,并导致前导激波波阵面上压力峰值逐渐出现在30°方向上。     

Changes in radio emission from PSR J0737–3039B

The double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.     

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.     

GPS接收机天线相位中心变化对基线解的影响

GPS接收机天线相位中心变化与卫星信号的入射方向有关，因此相位中心变化对基线解的影响还与参加解算的卫星个数及卫星的几何分布有关。在考虑卫星几何分布情况下，首先研究了相位中心变化对单个点位坐标的影响，然后推导了相位中心变化引起的基线矢量的偏差计算公式。此计算公式综合考虑了各种引起天线相位中心变化的因素，如天线的类型、天线的安置误差、卫星的几何分布、卫星个数等。最后，给出了具体算例，并给出了减弱这种影响的方法。     

论中国金融风险问题

文章结合国内金融市场的发展和国际金融市场的大趋势，阐述了中国金融风险突出的种种原因，进一步提出了防范和化解金融风险的有效对策。     

矩阵方程（AX，XB）=（C，D）和AXB=C的对称正定解

讨论了矩阵方程（ＡＸ，ＸＢ）＝（Ｃ，Ｄ）和ＡＸＢ＝Ｃ的对称正定解。利用奇异值分解和广义奇异值分解导出了这些矩阵方程有对称正定解的充分必要条件，并且给出了一般对称正定解的表达式     

组合荷载作用下非完善层合板后屈曲分析的半解析法

本文采用经典层合板理论，研究横向荷载作用下面内受压非完善复合材料层合板的后屈曲问题。分析中将板在横向荷载作用下产生的小挠度弯曲变形和几何缺陷视为结构的初始挠度，给出了基于摄动技术、单向DQ离散格式和Galerkin法的半解数值分析方法，可方便地分析不同边界约束（简支、固支、弹性转动约束等）层合板的后屈曲性态。文中通过算例讨论了边界约束、荷载型式、纤维铺设方式等因素层合板后屈曲行为的影响。