自动测试系统通用性的实现技术

文章分析了与开发通用ATS密切相关的标准/规范,从软、硬件两方面讨论了ATS通用性的实现途径,包括硬件配置及接口技术、IVI技术以及面向信号方法。ATS通用性的实现可以实现被测对象的跨平台测试以及测试程序的可移植,能带来显著的军事及经济效益。     

新型高低速流统一算法及其叶轮机应用

 对于可压缩/不可压缩混合流动或高低速混合流动问题,目前没有较好的解决方法。基于Roe格式及预处理方法,提出了全速度Roe格式。全速度Roe格式是将Roe格式与低速Roe格式通过一个与本地马赫数相关的函数联合而得到的。与标准Roe格式相比,对亚音速流动,全速度Roe格式中声速对数值耗散的影响随着马赫数变化而变化。与预处理Roe格式相比,全速度Roe格式简单易于实现,而且没有计算稳定性的限制,不需要采用全局截断处理,从而在理论上对高低速流动具有一致精度。事实上,全速度Roe格式意味着可以通过直接改变Roe格式的非线性特征值,解决可压不可压流动统一计算精度的问题。这是对统一算法的新观点。数值模拟表明,全速度Roe格式具有与预处理Roe格式一样的激波捕获能力、极低速流动准确模拟能力。     

有限扫描反射面天线纵向偏焦性能的研究

随着相控阵天线的不断发展,有限扫描反射面天线已经成为当前的研究热点,为了符合新时代天线多功能的需求,提出一种基于抛物面形变的纵向偏焦特性。设计一个标准正馈反射面天线,使其馈源固定不动,而利用调节反射面焦距来达成天线的偏焦,其偏焦特性类似于抛物面天线的纵向偏焦特性;设计一个双焦点反射面,由XOZ平面抛物线和YOZ平面抛物线正交互异设计双焦点反射面天线,令YOZ平面抛物线焦点外推、XOZ平面抛物线焦点不变构成一个双焦点反射面。验证了该方法在一维阵列作为馈源的有效性,双焦点反射面相较于标准抛物面,在EL方向上该天线增益上升了14.29dB,且波束宽度基本不变;此外,该方法还能容纳所有馈源同时工作,降低了单个馈源喇叭的功率且增益相较于点波束天线只下降了4.85dB。该方法将为后续有限扫描反射面天线在设计一维扫描或二维不等范围扫描提供理论支撑。     

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。     

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.     

导弹落点密集度的序贯截尾决策

利用后退归纳法讨论了截尾情况下导弹落点密集度的序贯决策方案 ,给出了确定最优停时的一般方法 ,仿真结果表明了方法的有效性     

逆向卸荷式气体减压阀的动态特性仿真

考虑到摩擦力、阻尼力及流体流动作用力等主要非线性因素对减压阀动态特性的影响,建立了逆向卸荷式气体减压阀的动态特性数学模型,并对其启动过程与负载变化下的动态响应特性进行了仿真计算,研究了动态过程的压力、温度、流量以及阀芯位移等参数变化情况,分析了不同的参数对减压阀启动特性的影响,提出了改善减压阀动态响应特性的措施。     

Reducing mission operations costs through spacecraft autonomy: the near earth asteroid rendezvous (near) experience

With a maximum time of 12 days out of ground contact and a round-trip light time as high as 56 minutes, The Near Earth Asteroid Rendezvous (NEAR) spacecraft requires a moderate degree of onboard autonomy to react to faults and safe the spacecraft. Beyond the basic safing requirements, additional functions are carried out onboard. For example, on-board calculation of the Sun, Earth, asteroid, and spacecraft positions allow the spacecraft to autonomously orient itself for science and downlink operations. On-board autonomous momentum management during cruise relieves Mission Operations from planning, scheduling, and carrying out many manual momentum dumps. During development, additional operations, such as center-of-mass management during propulsive maneuvers and optical navigation were also considered for onboard autonomy on the NEAR spacecraft, but were not selected. The allocation of functions to onboard software or to ground operations involved tradeoffs such as development time for onboard software versus ground software, resource management, life cycle costs, and spacecraft safety.After two years of cruise operations, considerable experience with the NEAR autonomy system has accrued. The utility of some autonomous capabilities is greater than expected, others less so. Software uploads increased spacecraft autonomy in some cases, and the impact on Mission Operations can be assessed. Allocation of functions between spacecraft autonomy and ground operation during development of future missions can be improved by applying the lessons learned from the NEAR experience.