铝合金T型材拉弯成形的有限元模拟

针对目前拉弯成形中的问题,采用有限元模拟的方法,对带下陷拉弯过程进行计算机仿真,得到优化后的工艺参数,避免了盲目的试拉,提高了加工效率,降低了拉弯成本,积累了带下陷拉弯成形的经验,提高了公司拉弯工艺水平。     

利用模拟试验研究APC预测准则的适应性

使用多种飞机系统构型的人机耦合(APC)振荡地面模拟试验数据,研究各种Ⅰ类、Ⅱ类APC预测准则的适用性,通过对比分析试验中试飞员评分结果和各种准则计算结果,得到APC预测准则与试飞员APC趋势评分的符合率。研究结果表明,现有的APC预测准则并非预想的那样有效,进而针对APC预测准则和模拟试验提出改进建议。     

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).     

面向对象技术的防空导弹Simulink建模与仿真

为防空导弹系统性能改进研究和优化设计,提出了一种新的方法,首先给出了一般防空导弹制导控制系统的数学模型,并采用面向对象建模技术结合动态仿真软件Simulink建立了仿真模型并进行了仿真研究,该模型具有容易理解,可重复使用,易于扩展等优点,即通过部分模块更换或改变参数等就可对该系统在其他条件下进行仿真,仿真结果和实际遥测数据基本吻合,表明了该模型和方法的有效性和实用性。     

转发式干扰下GPS定位精度的仿真分析

根据GPS转发式干扰的原理,建立了转发式干扰对GPS定位精度影响的数学模型.讨论了两种转发式干扰模式对定位的影响.最后通过计算机仿真分析得出了GPS转发式干扰对GPS定位精度影响的相关结论.     

计算风工程中几个关键影响因素的分析与建议

通过近几年进行建筑计算风工程的实践与体会,并参考国内外的一些文献,本文给出了合理选取建筑数值风洞大小、最好采用SSTk-ω或BSL雷诺应力湍流物理模型及在建筑模型中的不同区域应按不同的网格尺度要求划分网格的建议;在CFX5软件平台中,对复杂的建筑体型,可选用非结构化网格和四面体单元,对流项的插值格式宜采用接近二阶的混合格式。还选取一立方体建筑模型,通过数值模拟、现场实测和风洞实验结果的比较对建议进行了验证。最后通过未受扰动数值风洞中入口边界条件的保持,给出了适用于我国建筑工程中A、B、C、D四类地面粗糙度类别的入口湍流边界条件,可参考采用。     

虚拟环境系统中复杂模型的建立--3D资源在快速开发虚拟环境系统中的应用

对利用3D资源在快速开发虚拟环境系统中的方法进行了研究。在开发虚拟环境系统的过程中，复杂模型的建立是必不可少的，仅仅利用OpenGL函数编程来实现仿真是很困难的，针对该问题提出了利用3D资源进行3D文件读取和转换的两种方案，分析了虚拟环境中复杂模型的建立以及处理的基本方法，并对数控车床的仿真进行了详细介绍。     

Grid-Adaptive Computations of Magnetized Jets

We present grid-adaptive numerical simulations of magnetized plasma jets, modeled by means of the compressible magnetohydrodynamic equations. The Adaptive Mesh Refinement strategy makes it possible to investigate long-term jet dynamics where both large-scale and small-scale effects are at play. We extend recent findings for uniformly magnetized, periodic shear layers to planar and fully 3D extended jet segments. The jet lengths cover multiple, typically 10, axial wavelengths of the fastest growing Kelvin–Helmholtz (KH) like modes. The dominant linear MHD instabilities of the jet flows are quantified by means of MHD spectroscopic analysis. In cases characterized by sonic Mach numbers about unity and large plasma beta values, both single and double shear layers (planar jets) manifest self-organizing trends to large scales, e.g. by continuous pairing/merging between co-rotating vortices, simultaneously with the introduction of small-scale features by magnetic reconnection events. The vortices form as a result of KH unstable shear-flow layers, and their coalescence arises from the growth of subharmonic modes at multiple wavelengths of the fastest growing KH instability. In extended two-dimensional jet segments, we investigate how varying jet width alters this coalescence process occurring at both edges, e.g. by introducing Batchelor-like coupling between counter-rotating vortices formed at opposing weakly magnetized, close shear layers. Finally, periodic segments of supersonic magnetized jets are simulated in two- and three-dimensional cases, which are characterized by violent shock-dominated transients.     

俯仰轴飞行品质中频域准则的计算与模拟

简要介绍了军用飞机飞行品质MIL—STD—1797A中有关俯仰轴频域难则的要求和原由。提出了对这些难则的理论计算和模拟试验方法。并以某飞机为例，利用所提出的方法，对其飞行品质进行了计算和模拟。结果表明，所提出的计算和模拟方法是合理的。最后，讨论了驾驶员模型形式对俯仰轴飞行品质的影响。     

A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind Simulations

It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.