Inverse identification of constitutive parameters of Ti2AlNb intermetallic alloys based on cooperative particle swarm optimization

Ti₂AlNb intermetallic alloy is a relatively newly developed high-temperature-resistant structural material, which is expected to replace nickel-based super alloys for thermally and mechanically stressed components in aeronautic and automotive engines due to its excellent mechanical properties and high strength retention at elevated temperature. The aim of this work is to present a fast and reliable methodology of inverse identification of constitutive model parameters directly from cutting experiments. FE-machining simulations implemented with a modified Johnson-Cook (TANH) constitutive model are performed to establish the robust link between observables and constitutive parameters. A series of orthogonal cutting experiments with varied cutting parameters is carried out to allow an exact comparison to the 2D FE-simulations. A cooperative particle swarm optimization algorithm is developed and implemented into the Matlab programs to identify the enormous constitutive parameters. Results show that the simulation observables (i.e., cutting forces, chip morphologies, cutting temperature) implemented with the identified optimal material constants have high consistency with those obtained from experiments, which illustrates that the FE-machining models using the identified parameters obtained from the proposed methodology could be predicted in a close agreement to the experiments. Considering the wide range of the applied unknown parameters number, the proposed inverse methodology of identifying constitutive equations shows excellent prospect, and it can be used for other newly developed metal materials.     

Identification of seismic activity sources on the subsatellite track by ionospheric plasma disturbances detected with the Sich-2 onboard probes

Using a cylindrical Langmuir probe and the authors’ proprietary two-channel pressure transducer, ionospheric plasma parameter distributions along the orbit of the Sich-2 satellite (Ukraine, 2011–2012) were measured. This paper is concerned with identifying the space–time location of ionospheric plasma disturbance sources, including the epicenters of actual earthquakes (before or during the satellite flyover) and incipient earthquakes on the subsatellite track, from the measured distributions of the electron density and temperature and the neutral particle temperature along the satellite orbit. To do this, the measured ionospheric plasma parameter distributions are connected to the coordinates on the subsatellite track.It is shown that local disturbances in the electron density and temperature and neutral particle temperature distributions in the satellite orbit in the ionosphere may serve as indicators of seismic activity on the subsatellite track. The epicenters of incipient earthquakes may be set off from other plasma parameter disturbance sources associated with seismic activity using information provided by special monitoring and survey centers that monitor the current seismic situation.     

A drilling tool design and in situ identification of planetary regolith mechanical parameters

The physical and mechanical properties as well as the heat flux of regolith are critical evidence in the study of planetary origin and evolution. Moreover, the mechanical properties of planetary regolith have great value for guiding future human planetary activities. For planetary subsurface exploration, an inchworm boring robot (IBR) has been proposed to penetrate the regolith, and the mechanical properties of the regolith are expected to be simultaneously investigated during the penetration process using the drilling tool on the IBR. This paper provides a preliminary study of an in situ method for measuring planetary regolith mechanical parameters using a drilling tool on a test bed. A conical-screw drilling tool was designed, and its drilling load characteristics were experimentally analyzed. Based on the drilling tool-regolith interaction model, two identification methods for determining the planetary regolith bearing and shearing parameters are proposed. The bearing and shearing parameters of lunar regolith simulant were successfully determined according to the pressure-sinkage tests and shear tests conducted on the test bed. The effects of the operating parameters on the identification results were also analyzed. The results indicate a feasible scheme for future planetary subsurface exploration.     

电视遥控制导武器深入测试研究与应用

介绍了电视遥控制导武器的原理及其在航电综合试验中存在的问题，给出了对电视遥控制导武器进行深入测试的方法，论述了该方法应用到飞机平台中作为嵌入式训练系统的技术可行性。     

基于新陈代谢GM（1,1）模型的导弹遥测故障预测算法

在人工监视遥测关键参数是否超出阈值范围以判断导弹故障的传统模式基础上,对GM（1,1）预测模型进行了改进,研究了基于新陈代谢的GM（1,1）预测算法对遥测参数实时预测效果.该算法能不断去掉最老的信息,充分利用最新的信息,避免了预测模型老化的现象;由于用于预测的数列维度较少,便于计算,能够保证算法的实时性.用MATLAB编程实现算法,比对实测数据的预测值与实际值,并进行误差分析.结果表明,该算法对遥测参数的预测精度较高,可为及时发现导弹故障提供科学的依据.     

钛合金TC4的超硬磨料柔性抛光轮数控抛光试验研究

航空发动机叶片钛合金材料在数控磨抛加工中容易发生烧伤及黏附现象,针对常用的TC4材料开展了超硬磨料柔性抛光轮数控抛光试验研究。分析了超硬磨料柔性抛光轮抛光参数中转速、进给速度、预压量及行距对抛光去除深度及抛光后试件表面粗糙度的影响规律并通过正交试验分析了各抛光参数影响的主次关系。确认了钛合金试件抛光表面黏附物质成分,并同时分析了表面黏附物的形成原理。给出了TC4钛合金材料在超硬磨料柔性抛光轮数控抛光过程中工艺参数的选择策略,为TC4材料的航空发动机叶片和整体叶盘在超硬磨料柔性抛光轮数控抛光过程中提供理论依据和技术基础。     

织物细观结构参数对编织复合材料弹性性能的影响

根据作者提出的二维波纹细观力学模型,在考虑了实际织物结构中存在的经向和纬向纤维的波纹;相邻纤维束之间的间隙;纤维束的横截面尺寸和织物的叠层构造状态对编织复合材料弹性性能的影响下,给出了织物细观结构参数与编织复合材料弹性性能之间的变化关系。通过参数分析探讨了不同结构参数对编织复合材料弹性性能的影响。     

线性时不变系统的完全跟踪控制器

从线性时不变系统的状态空间模型出发,借助于广义逆矩阵概念和相容线性方程组的最小范数解,从理论上推导了线性时不变系统的完全跟踪控制器方案。     

激光辅助车削工艺参数对单晶硅表面质量的影响

为了提高单晶硅激光辅助车削加工表面质量,通过开展激光辅助和常规车削加工试验,结合表面粗糙度、表面形貌及拉曼光谱检测,研究激光辅助车削技术对加工质量的影响。基于正交试验方法,研究单晶硅激光辅助车削工艺参数对表面粗糙度的影响;通过方差分析和极差分析评估各因素对表面粗糙度的影响。研究结果表明：与常规车削相比,激光辅助车削可有效提高加工表面质量,降低材料表面的残余应力。主轴转速、进给速度、切削深度和脉冲占空比对表面粗糙度的贡献率分别为17.51%、44.48%、6.69%和14.70%。确定最佳加工参数组合如下：主轴速度为4 000 r/min,进给速度为2 mm/min,切削深度为5μm,脉冲占空比为30%,最终获得表面粗糙度Rq为2.4 nm的高质量表面。     

轨道参数对阿尔法磁谱仪太阳辐射热流的影响

为探明阿尔法磁谱仪（AMS）的温度变化规律,并为制定AMS的热控制方案提供指导和依据,推导了AMS重要区域（AMS前方、后方、顶部和左舷）的太阳辐射热流计算公式,分析了这些区域太阳辐射热流随轨道参数的变化,解释了AMS顶部的温度变化和太阳辐射热流变化规律在热控方案中的应用。分析表明在国际空间站（ISS）正常飞行姿态下,AMS前、后方和左舷的太阳辐射热流受太阳光与ISS轨道面的夹角（β角）、ISS与会日点的角距（θ角）和地球阴影区的影响,AMS顶部太阳辐射热流受β角和θ角的影响。得出结论：β角、θ角和地球阴影区均是影响AMS温度的主要因素,各区域的太阳辐射热流变化规律可以作为设计AMS温度控制方案的主要依据之一。