大飞机货舱地板下部结构有限元建模与适坠性分析

为了研究大飞机坠撞特性及数值分析方法，选取大飞机货舱地板下部结构为研究对象，建立其有限元模型，实现显式动力学的求解与分析。考察倒置、固支的货舱地板下部结构在200 kg落重以7 m/s垂直冲击下的结构响应、吸能与失效的动态行为，识别落重冲击过程中结构变形与失效模式、冲击响应特性及能量吸收与耗散机理。仿真结果表明，货舱地板下部结构的机身框组件、支撑件组件是主要吸能结构，冲击能量的吸收主要依靠上述结构的塑性变形与失效，紧固件的吸能贡献仅占1%左右。     

Depth dependency of neutron density produced by cosmic rays in the lunar subsurface

Depth dependency of neutrons produced by cosmic rays (CRs) in the lunar subsurface was estimated using the three-dimensional Monte Carlo particle and heavy ion transport simulation code, PHITS, incorporating the latest high energy nuclear data, JENDL/HE-2007. The PHITS simulations of equilibrium neutron density profiles in the lunar subsurface were compared with the measurement by Apollo 17 Lunar Neutron Probe Experiment (LNPE). Our calculations reproduced the LNPE data except for the 350–400 mg/cm² region under the improved condition using the CR spectra model based on the latest observations, well-tested nuclear interaction models with systematic cross section data, and JENDL/HE-2007.     

任意多面体网格上的欧拉方程数值算法

发展并验证了一种新的支持多面体网格的欧拉方程离散算法,采用Fortran 95编写了支持任意网格拓扑及三维复杂外形的通用求解器.在空间离散上,基于径向基函数理论提出了一种新的梯度计算方法,并采用动能通量分裂格式来得到准确并且稳定的二阶精度重构.该方法不依赖于网格几何形状,因此对网格质量不敏感.由于在时间方向采用了点隐松...     

平面磨削石英陶瓷比磨削能正交试验研究

通过大量的正交试验,研究陶瓷材料在低速下的磨削性能,优化陶瓷磨削参数,对于丰富陶瓷磨削理论,指导实际生产实践具有重要的现实意义.     

基于能量法的舰载机拦阻着舰动力学分析及建模仿真

针对舰载机拦阻着舰过程,采用能量法分析了任意着舰姿态和位置下的拦阻力响应,建立了全机六自由度动力学模型,考虑了航母甲板风的影响以及航母纵摇和升沉运动。通过MATLAB／SIMULINK建立数学模型,并以一种偏心非垂直着舰拦阻状态为算例进行了仿真分析。     

火箭发动机胶接质量检测的兰姆波能量分布研究

用兰姆波可对固体火箭发动机进行胶接质量的检测,但需要对其模式进行选择。通过研究兰姆波在固体发动机钢壳体内纵波与横波成分的能量分布情况,从理论上分析和预测了不同模式对检测特定界面缺陷的能力和灵敏度,并通过S0和S1两种检测模式的试验研究,验证了理论分析的正确性。结果表明,可根据兰姆波的能量分布变化特性和实际检测要求,选择最合适的模式进行检测,从而达到提高界面缺陷检测灵敏度的目的。     

新一代运载贮箱搅拌摩擦焊应用研究

在分析搅拌摩擦焊(FSW)原理和工艺特点的基础上,设计了适于厚6 mm 2219铝合金焊接用搅拌头,进行了平板工艺试验,以及焊缝的外观质量、金相组织和力学性能评定。采用线能量因子确定了最佳工艺容限。新一代运载2219铝合金贮箱1∶1验证件的焊接和压力试验证明,FSW的焊接质量、构件整体尺寸精度和生产效率都远高于传统的交流钨极惰性气体保护焊(TIG),完全满足新一代运载贮箱的制造要求。     

？ET／N100粘合剂体系固化过程的DSC研究

采用高压DSC方法，研究了PET／N100粘合剂体系的固化过程，获得了该体系的动力学参数及反应机理函数，并比较了不同添加物对体系动力学参数的影响。结果表明，PET／N100固化体系的反应机理函数符合g（a）=-In（1-a）；为一级反应；固化反应机理函数不受各种添加物的影响，动力学参数受这些添加物的影响而发生变化。     

Locating Current Sheets in the Solar Corona

Current sheets are essential for energy dissipation in the solar corona, in particular by enabling magnetic reconnection. Unfortunately, sufficiently thin current sheets cannot be resolved observationally and the theory of their formation is an unresolved issue as well. We consider two predictors of coronal current concentrations, both based on geometrical or even topological properties of a force-free coronal magnetic field. First, there are separatrices related to magnetic nulls. Through separatrices the magnetic connectivity changes discontinuously. Coronal magnetic nulls are, however, very rare. Second, inspired by the concept of generalized magnetic reconnection without nulls, quasi-separatrix layers (QSL) were suggested. Through QSL the magnetic connectivity changes continuously, though strongly. The strength of the connectivity change can be quantified by measuring the squashing of the flux tubes which connect the magnetically conjugated photospheres. We verify the QSL and separatrix concepts by comparing the sites of magnetic nulls and enhanced squashing with the location of current concentrations in the corona. Due to the known difficulties of their direct observation, we simulated coronal current sheets by numerically calculating the response of the corona to energy input from the photosphere, heating a simultaneously observed Extreme Ultraviolet Bright Point. We did not find coronal current sheets at separatrices but at several QSL locations. The reason is that, although the geometrical properties of force-free extrapolated magnetic fields can indeed hint at possible current concentrations, a necessary condition for current sheet formation is the local energy input into the corona.     

飞行器结构力学中的一个问题

最小余能原理的丰富内涵在飞行器结构力学中得到一定反映。研究了飞行器结构力学中余虚功原理的两种不同的表示形式，最小余能原理和拟余能原理，推导了最小余能原理驻值条件。最后，给出典型实例。