基于LabVIEW设计曲线拟合仪

基于LabVIEW图形化编程环境和软件分析库函数设计的曲线拟合仪，界面友好，功能齐全，操作简便，在科学研究和工程应用中具有较强的实用价值。文中简要介绍利用NI虚拟仪器技术设计曲线拟合仪的方法，给出软件设计思想与实现方案，对主要软件功能模块进行了分析。     

The Origin of Mercury

Mercury’s unusually high mean density has always been attributed to special circumstances that occurred during the formation of the planet or shortly thereafter, and due to the planet’s close proximity to the Sun. The nature of these special circumstances is still being debated and several scenarios, all proposed more than 20 years ago, have been suggested. In all scenarios, the high mean density is the result of severe fractionation occurring between silicates and iron. It is the origin of this fractionation that is at the centre of the debate: is it due to differences in condensation temperature and/or in material characteristics (e.g. density, strength)? Is it because of mantle evaporation due to the close proximity to the Sun? Or is it due to the blasting off of the mantle during a giant impact? In this paper we investigate, in some detail, the fractionation induced by a giant impact on a proto-Mercury having roughly chondritic elemental abundances. We have extended the previous work on this hypothesis in two significant directions. First, we have considerably increased the resolution of the simulation of the collision itself. Second, we have addressed the fate of the ejecta following the impact by computing the expected reaccretion timescale and comparing it to the removal timescale from gravitational interactions with other planets (essentially Venus) and the Poynting–Robertson effect. To compute the latter, we have determined the expected size distribution of the condensates formed during the cooling of the expanding vapor cloud generated by the impact. We find that, even though some ejected material will be reaccreted, the removal of the mantle of proto-Mercury following a giant impact can indeed lead to the required long-term fractionation between silicates and iron and therefore account for the anomalously high mean density of the planet. Detailed coupled dynamical–chemical modeling of this formation mechanism should be carried out in such a way as to allow explicit testing of the giant impact hypothesis by forthcoming space missions (e.g. MESSENGER and BepiColombo).     

Modelling of Ejecta as a Space Debris Source

When a micro-debris or a micrometeoroid impacts a spacecraft surface, a large number of secondary particles, called ejecta, are produced. These particles can contribute to a modification of the debris environment: either locally by the occurrence of secondary impacts on the components of complex and large space structures, or at great distance by the formation of a population of small orbital debris. This paper describes firstly, the ejecta overall production, and secondly, the lifetime and the orbital evolution of the particles. Finally the repartition of ejecta in LEO is computed. Some results describing the population as a function of size and altitude are presented.     

空战机动动作库设计方式研究

具体阐述了两类常见空战动作库的设计 :典型战术动作库和基本操作动作库 ,详细分析了这两类空战机动动作库的不足 ,最后提出了改进动作库设计的具体意见和建议。     

低空突防任务下综合飞行/推进系统的建模与仿真

建立了综合飞行／推进系统的数学模型，介绍了飞机全维非线性数学模型和涡轮风扇发动机非线性部件级数学模型的建模及综合方法。对飞机执行地形中随任务时，飞行员调节飞行速度的方法与基于总能量的调节飞行速度的方法进行了比较。结果表明，基于总能量的方法比飞行员直接控制飞行速度能够减小发动机的燃油消耗，降低发动机的磨损，进而可以增加飞机的航程，延长发动机的使用寿命。     

四维下降飞行技术的研究与仿真：定常航迹角法下降剖面解算

本文研究的是四维飞行性能管理系统的核心环节－飞机在终端区域内的四维下降技术，首先探讨了基于常值航迹角的定常Ｍ数／指示空速下降飞行技术，论述了其高度剖面的构成与特点，通过尤拉积分方法求解飞机运动方程，实现了高度冲面的解算。其次开发了对速度剖面的迭代过程，选取原则及方法。本文在进行理论分析的同时，还开发了满意的仿真软件，一了其应用价值。     

星载遥感器在模拟空间环境中辐射定标设备研制

文章简述了星载遥感器辐射定标设备的研制过程及其在模拟空间环境中的调试过程,试验证明了该设备设计的合理性。     

磁粉检验标准环形试块的机理分析

为了分析控制磁粉检验系统综合性能的标准环形试块的机理，首先建立一个计算漏磁场的简化数学模型，然后解标量磁位的=维拉普拉斯方程，求出被磁化的环形试块上圆孔产生的漏磁场，计算环形试块表面的磁粉受力，分析其特点并得出相应的结论。     

尾支杆干扰非线性修正方法的初步研究

利用CFD方法 ,采用两套网格重叠的形式 ,研究了一种对尾支杆干扰进行修正的非线性方法。运用本方法 ,研究了尾支杆等直段长度、直径和锥角对模型气动特性的影响 ,研究了四个模型有攻角时的尾支杆干扰 ,并对GBM 0 4A模型的零阻进行了尾支杆干扰的修正。     

大客车局部优化造型对其使用性能的影响

随着车速的提高,汽车在行驶中受到的空气阻力便成为不可忽视的问题,因此与减阻节能相关的汽车优化造型也就显得越来越重要了。由于运动物体所受到的空气阻力系数的大小主要取决于它的头部的形状,因而我们对厢式大客车驾驶室前风窗区的几种不同造型在低速风洞中进行了测力的实验研究。实验结果表明,驾驶室前围不同形式的过渡是影响厢式客车空气阻力的重要因素。其中在适当的风窗倾角下,经过良好的圆化处理后,可使厢式大客车的空气阻力减小27%左右。这不仅节省了燃料的消耗,还可以提高汽车的最大行驶速度,改善其加速和爬坡能力。