镁合金微弧氧化膜的相结构研究

针对镁合金微弧氧化膜层,对其相组成和品粒尺寸随工艺参数的变化规律进行了定件和定量分析,并考察了相组成对膜层耐蚀性能的影响.结果表明:不同工艺参数条件下制备的微弧氧化膜层均由镁铝尖晶石和方镁石两相组成,但两相的含量差别很大.当这两相含量的比值在0.6～1.0范围内时,膜层的耐蚀性明显提高.不同时间内制备的膜层中MgAl2O3晶粒尺寸都在40～50nm的范围内,随着氧化时间的增加,晶粒尺寸呈现先减小后增大的趋势.     

A novel unified model predicting flow stress and grain size evolutions during hot working of non-uniform as-cast 42CrMo billets

The cast preformed forming process(CPFP) is increasingly considered and applied in the metal forming industries due to its short process, low cost, and environmental friendliness, especially in the aerospace field. However, how to establish a unified model of a non-uniform as-cast billet depicting the flow stress and microstructure evolution behaviors during hot working is the key to microstructure prediction and parameter optimization of the CPFP. In this work, hot compression tests are performed using a non-uniform as-cast 42 CrMo billet at 1123–1423 K and 0.01–1sà1. The effect laws of the non-uniform state of the as-cast billet with different initial grain sizes on the flow stress and microstructure are revealed deeply. Based on experimental results, a unified model of flow stress and grain size evolutions is developed by the internal variable modeling method. Verified results show that the model can well describe the responses of the flow stress and microstructure to deformation conditions and initial grain sizes. To further evaluate its reliability, the unified model is applied to FE simulation of the cast preformed ring rolling process.The predictions of the rolling force and grain size indicate that it could well describe the flow stress and microstructure evolutions during the process.     

PIV测速技术实验参数分析

本文通过理论分析、计算机模拟及实验观测，对采用底片记录和杨氏条纹法判读的ＰＩＶ测速技术的动态测量范围、各种实验参数的影响及其优化取值准则进行了详细的分析讨论，并给出了一些有关的理论及经验公式。     

某型无人机起落架放下阶段缓冲器气液流动特性研究

在设计飞机油气混合型式的可收放起落架时,应充分考虑其内腔之间的介质流动特性。以某型无人机起落架缓冲器阻尼孔径、充油量为研究对象,采用单因素实验法对各因素引起的缓冲器内部气液流动变化进行分析,通过Fluent软件对放下阶段不同阻尼孔径、充油量下的缓冲器气液特性进行仿真计算。结果表明：起落架放下过程缓冲器阻尼孔油液流量只与孔径大小有关,不受缓冲器充油量影响;在该型号无人机要求的637 mL充油量下,缓冲器阻尼孔孔径应大于6 mm;对于其他型号起落架缓冲器,当确定了充油量后,应将满足放下阶段缓冲器气液充填作为缓冲器阻尼孔设计标准之一。     

粒子激发X射线谱仪的热设计和热仿真计算

粒子激发X射线谱仪(APXS)安装在月面巡视器外部,利用巡视器的机动性和机械臂的灵活性,可以对月面有研究价值的月岩及月壤进行有针对性的探测.由于裸露在巡视器外部,月球复杂外热流会对APXS产生较大影响.鉴于此,需对APXS进行合理的热设计,以保证APXS的探测器和电子学器件工作在允许的温度范围内.提出了APXS的热设计方案,据此对APXS进行热仿真计算,计算结果得到了相应热平衡试验的较好验证.     

高密度粒子场全息测试中粒子间相互作用的研究

本文用圆盘粒子模型对粒子场中粒子间相互作用作了定量计算,得出高密度粒子场中的大粒子效应及全息记录中的全息图效应等结论,由于这些效应的存在,使得在分析处理粒子场时,会出现小粒子丢失,从而给粒子场的统计分布特性分析提供了重要的理论依据。     

一种带宽扩展的小型化微带天线

设计了一种中心频率位于S波段、结构简单的单层微带贴片天线。一方面,通过在贴片表面加载变形的Sierpinski分形槽,使天线的谐振频率降低了287 MHz,实现了贴片尺寸的缩减;另一方面,在天线接地面上加载地面缺损结构(DG S),通过优化DGS在接地面上的布局,当天线工作在2.4 GH z时,RVSW(电压驻波比)≤2.0的绝对带宽有219MHz,比不加DG S的同类天线提高了3倍多。综合应用上面两种技术后,加载DG S的小型化天线的绝对带宽也有174 MHz,达到了缩减天线尺寸和带宽扩展的双重效果。     

多普勒辅助测量IMM-PF机动目标跟踪

针对机动目标跟踪问题,提出了一种辅助多普勒测量的交互多模型粒子滤波算法.该算法利用粒子滤波解决系统观测与目标状态之间的非线性问题,并辅助多普勒测量信息在线估计目标角速率,作为目标转弯模型的参数.采用两个可内部切换的运动模型(常速度/逆时针转弯模型、常速度/顺时针转弯模型)作为交互模型,有效地描述了目标机动并减少了模型个数,进一步提高了算法的效率.对一个以不同角速率多次转弯的机动目标进行跟踪仿真,结果验证了算法的可行性和优越性.     

基于SMC-CPHD的多目标跟踪算法研究

针对CPHD滤波算法在多目标跟踪中计算难处理和对于局部目标估计存在漏检的问题,提出了基于序贯蒙特卡罗方法的基数概率假设密度（SMC-CPHD）滤波算法。这种方法是将SMC和CPHD两种滤波算法的优点相结合,用一些离散的粒子去接近PHD函数,不仅解决了在滤波修正步没有闭式解的问题,而且避免了当某个目标发生漏检时,PHD权值的转移问题,在递推PHD函数的同时也递推基数分布。将此方法应用到有杂波存在复杂的多目标跟踪环境中,通过仿真实验,对CPHD滤波和SMC-CPHD滤波得出的结果进行比较,验证了本文所提出方法对多目标跟踪的可行性和精确性。     

Advanced data acquisition system for SEVAN

Huge magnetic clouds of plasma emitted by the Sun dominate intense geomagnetic storm occurrences and simultaneously they are correlated with variations of spectra of particles and nuclei in the interplanetary space, ranging from subtermal solar wind ions till GeV energy galactic cosmic rays. For a reliable and fast forecast of Space Weather world-wide networks of particle detectors are operated at different latitudes, longitudes, and altitudes. Based on a new type of hybrid particle detector developed in the context of the International Heliophysical Year (IHY 2007) at Aragats Space Environmental Center (ASEC) we start to prepare hardware and software for the first sites of Space Environmental Viewing and Analysis Network (SEVAN). In the paper the architecture of the newly developed data acquisition system for SEVAN is presented. We plan to run the SEVAN network under one-and-the-same data acquisition system, enabling fast integration of data for on-line analysis of Solar Flare Events. An Advanced Data Acquisition System (ADAS) is designed as a distributed network of uniform components connected by Web Services. Its main component is Unified Readout and Control Server (URCS) which controls the underlying electronics by means of detector specific drivers and makes a preliminary analysis of the on-line data. The lower level components of URCS are implemented in C and a fast binary representation is used for the data exchange with electronics. However, after preprocessing, the data are converted to a self-describing hybrid XML/Binary format. To achieve better reliability all URCS are running on embedded computers without disk and fans to avoid the limited lifetime of moving mechanical parts. The data storage is carried out by means of high performance servers working in parallel to provide data security. These servers are periodically inquiring the data from all URCS and storing it in a MySQL database. The implementation of the control interface is based on high level web standards and, therefore, all properties of the system can be remotely managed and monitored by the operators using web browsers. The advanced data acquisition system at ASEC in Armenia was started in November, 2006. The reliability of the multi-client service was proven by continuously monitoring neutral and charged cosmic ray particles. Seven particle monitors are located at 2000 and 3200 m above sea level at a distance of 40 and 60 km from the main data server.