基于四面体单元的三维裂纹自动化建模

三维裂纹前缘布置结构化网格是一项耗时且困难的工作。以二次四面体单元虚拟裂纹闭合法（VC‐CM）为基础,提出基于几何特征的三维裂纹建模方法,阐述应用四面体单元在ABAQUS上进行三维裂纹建模的实现细节;应用Python编程语言结合NumPy和SciPy开源科学计算库开发参数化三维裂纹分析程序包,实现三维裂纹问题分析的全流...     

多变量线性系统的特征模型及控制方法

对多输入 -多输出高阶线性定常系统从理论上详细推导出了其特征模型 ,并给出了基于特征模型的自适应模糊广义预测控制方案。所建立的特征模型为智能控制器设计和一些高阶对象的低阶控制器设计提供了理论依据 ,特别是为大型空间挠性航天器的控制提供了一种有效的途径。通过对一个航天器控制的仿真研究验证了所给方法的有效性     

某航空发动机机匣的动力学模型修正

利用动力学模型修正技术对某航空发动机机匣的有限元模型进行了修正.通过振动模态测试得到了实际机匣的模态数据用以作为有限元模型 修正的基准.利用频率对单元刚度的灵敏度分析选定了修正区域.在此基础上,应用1阶优化方法对机匣的有限元模型进行修正.研究结果表明:修正后机匣有限元模型的前10阶模态的计算值与实际测试的误差都在29%以内,可以应用在后续的发动机整机动力学分析等方面.      

Gravity Field Recovery from GRACE: Unique Aspects of the High Precision Inter-Satellite Data and Analysis Methods

The very high accuracy of the Doppler and range measurements between the two low-flying and co-orbiting spacecraft of the GRACE mission, which will be at the μm/sec and ≈10 μm levels respectively, requires that special procedures be applied in the processing of these data. Parts of the existing orbit determination and gravity field parameters retrieval methods and software must be modified in order to fully benefit from the capabilities of this mission. This is being done in the following areas: (i) numerical integration of the equations of motion (summed form, accuracy of the predictor-corrector loop, Encke's formulation): (ii) special inter-satellite dynamical parameterization for very short arcs; (iii) accurate solution of large least-squares problems (normal equations vs. orthogonal decomposition of observation equations); (iv) handling the observation equations with high accuracy. Theoretical concepts and first tests of some of the newly implemented algorithms are presented. This revised version was published online in August 2006 with corrections to the Cover Date.     

Reduction in clamping force due to applied longitudinal load to aerospace structural bolted plates

The main purpose of the present work is to experimentally and numerically study why and how the magnitude of the bolt clamping force reduces in the aerospace structural bolted plates when they are subjected to a longitudinal tensile load. In the experimental method, a holed plate of aluminium alloy 7075-T6 was clamped using a single bolt fastener, and then tested under an increasing static longitudinal tensile load. The bolt clamping magnitude was determined by using the measured axial compressive strains of a steel bush placed between the nut and plate. Two clamped specimens with different initial clamping forces were studied. In each specimen the actual clamping forces were determined during the longitudinal loading on the plate. In the numerical method, a three-dimensional (3D) finite element model was generated in order to simulate and quantify the bolt clamping force in the plate model loaded in tension. Both experimental and numerical results showed that the clamping force reduces considerably in the aluminium bolted plates under the longitudinal tensile loading. This is because of the transverse contraction of the plate material that causes the clamped material to release from the initial compression, and as a result, the clamping force to relax.     

一种新的串行离散事件仿真建模策略——信息驱动法

根据离散事件仿真的特点,提出了一种新的仿真建模方法,即信息驱动法。首先对仿真系统内的信息进行了分类,并介绍了各类信息的性质,然后说明了信息的接收与识别,信息对仿真系统的驱动作用,并给出了信息驱动法的执行结构。最后,用单服务排队系统说明信息驱动法的具体执行过程。     

ZL114A铝合金铸件显微孔隙的数值模拟

本文对ZL114A铝合金中显微孔隙的形成机理进行研究，介绍了孔隙率与二次枝晶的测量方法，考察了冷却速度对显微孔隙形成的影响，并提出了用冷却速度作为预测力学性能的判据。     

飞行模拟器建模、验模和性能测试与评估

仿真模型的精确度及仿真结果的置信度是飞行仿真系统研制中的关键和成功用于工程研究、人员培训的前提。主要介绍飞行模拟器仿真数学模型的特点,层次化、模快化建模方法,模型验证和性能测试与评估软件系统。     

基于改进粒子群的绳驱连续型机械臂逆运动学分析

绳驱连续型机械臂具有良好的柔性和灵活性,能够在狭小的空间内运动,但相对于离散型机械臂,利用D-H参数构建运动学模型的方法不再适用,且连续型机械臂具有无穷自由度,逆运动学求解困难。针对一种两节的绳驱连续型机械臂的运动学问题,基于分段常曲率假设,建立了运动学模型,并分析了两节之间的运动学耦合关系。在此基础上,利用改进粒子群优化算法求解连续型机械臂逆运动学,通过仿真验证了该逆解算法的可行性和有效性,搭建了绳驱连续型机械臂的物理样机系统,并验证了基于分段常曲率假设的正运动学模型的正确性。     

The response of the Hermean magnetosphere to the interplanetary magnetic field

The interaction between the solar wind and Mercury is anticipated to be unique because of Mercury’s relatively weak intrinsic magnetic field and tenuous neutral exosphere. In this paper the role of the IMF in determining the structure of the Hermean magnetosphere is studied using a new self-consistent three-dimensional quasi-neutral hybrid model. A comparison between a pure northward and southward IMF shows that the general morphology of the magnetic field, the position and shape of the bow shock and the magnetopause as well as the density and velocity of the solar wind in the magnetosheath and in the magnetosphere are quite similar in these two IMF situations. A Parker spiral IMF case, instead, produces a magnetosphere with a substantial north–south asymmetric plasma and magnetic field configuration. In general, this study illustrates quantitatively the role of IMF when the solar wind interacts with a weakly magnetised planetary body.