A three-dimensional plasma and energetic particle investigation for the wind spacecraft

This instrument is designed to make measurements of the full three-dimensional distribution of suprathermal electrons and ions from solar wind plasma to low energy cosmic rays, with high sensitivity, wide dynamic range, good energy and angular resolution, and high time resolution. The primary scientific goals are to explore the suprathermal particle population between the solar wind and low energy cosmic rays, to study particle accleration and transport and wave-particle interactions, and to monitor particle input to and output from the Earth's magnetosphere.Three arrays, each consisting of a pair of double-ended semi-conductor telescopes each with two or three closely sandwiched passivated ion implanted silicon detectors, measure electrons and ions above 20 keV. One side of each telescope is covered with a thin foil which absorbs ions below 400 keV, while on the other side the incoming <400 keV electrons are swept away by a magnet so electrons and ions are cleanly separated. Higher energy electrons (up to 1 MeV) and ions (up to 11 MeV) are identified by the two double-ended telescopes which have a third detector. The telescopes provide energy resolution of E/E0.3 and angular resolution of 22.5°×36°, and full 4 steradian coverage in one spin (3 s).Top-hat symmetrical spherical section electrostatic analyzers with microchannel plate detectors are used to measure ions and electrons from 3 eV to 30 keV. All these analyzers have either 180° or 360° fields of view in a plane, E/E0.2, and angular resolution varying from 5.6° (near the ecliptic) to 22.5°. Full 4 steradian coverage can be obtained in one-half or one spin. A large and a small geometric factor analyzer measure ions over the wide flux range from quiet-time suprathermal levels to intense solar wind fluxes. Similarly two analyzers are used to cover the wide range of electron fluxes. Moments of the electron and ion distributions are computed on board.In addition, a Fast Particle Correlator combines electron data from the high sensitivity electron analyzer with plasma wave data from the WAVE experiment (Bougeretet al., in this volume) to study wave-particle interactions on fast time scales. The large geometric factor electron analyzer has electrostatic deflectors to steer the field of view and follow the magnetic field to enhance the correlation measurements.     

铸造SiCp／ZL101复合材料的组织与性能

本文利用半固态搅拌铸造法制备了ＳｉＣｐ／ＺＬ１０１复合材料，对其组织和某些性能进行了研究，结果表明：ＳｉＣｐ在基体中分布均匀，无严重团聚现象，与基体结合良好，与基体合金相比，耐磨性，硬度有显著提高。     

直升机滑油换热器的结构优化设计

在直升机肋管式滑油换热器的初步热力性能设计计算基础上,应用数值优化原理,对滑油换热器结构的优化设计进行了研究,建立了结构优化程序.该程序以滑油换热器的重量为目标函数,采用正弦法去约束并结合单纯形加速法寻优.实例计算表明,将滑油换热器的热力性能计算程序同结构优化程序结合起来,可以建立自动匹配的换热器设计及优化程序系统.应用该软件,输入设计要求,就可获得既满足性能要求,且重量最轻的肋管式滑油换热器.该软件可推广应用于各种类型肋管式换热器.     

快速预热型铷原子振荡器的研制

介绍了一种快速预热型铷原子振荡器的设计方法和试验数据 ,3 5min的锁定时间、0 4 5L的小巧体积和良好的频率重现性能 ,非常适合于战术应用。     

飞机变形自动化测量方法研究

为解决以往飞机变形测量模式中人工干预较多,受测量环境影响较大,测量时间长等问题,基于Geo COM技术和RS232,在计算机与全站仪之间进行数据交换,设计了一套自动化测量系统。在测量过程中由标志点的机体理论坐标反算其在当前测站中的极坐标,从而在测量过程中驱动全站仪指向待测点,减少人工瞄准时间,并由计算机实时解算结果数据。经实际飞行试验验证表明,测量时间缩短为原来时间一半,大大提高了工作效率。     

双脉冲瞬态散斑全场测量方法研究CSCD

散斑测量技术在瞬态振动过程测量中具有不可或缺的重要地位。提出双脉冲瞬态散斑全场测量技术，解决了双脉冲激光器与双曝光相机的时序同步的关键技术，设计了基于双脉冲激光器的瞬态散斑光路系统，搭建了双脉冲瞬态散斑全场测量系统，从而实现了（2~800）μs 时间间隔内连续可调的瞬时振动形貌的测量。     

Crystal orientation and morphology of a lamellae in wrought titanium alloys: On the role of microstructure evolution in b processing

To obtain high-quality aviation forgings of titanium alloys, b forging is an essential processing step which must be considered throughout a production process. In this work, the effect of b forging on the crystal orientation and morphology of lamellar a was experimentally investigated in a two-phase titanium alloy. Strong dynamic recovery during b working resulted in the formation of low-angle grain boundary(LAGBb) inside b grains. The lamellar a can penetrate through the LAGBb, leading to similar intra a LAGBs on subgrain boundaries. Deformation banding occurs at high strain rates, and both diffusive and sharp boundaries of deformation bands can be observed.A continuous change of the b orientation in diffusive boundaries results in the formation of fine and disordered a lamellae without intra-lamellar boundary to hold the Burgers orientation relationship(OR). On sharp boundaries, it is prone to producing continuous grain boundary a(aGB) with a highly similar orientation along the boundaries. Meanwhile, there may exist several lower-angle boundaries within the grain boundary a for a smoother orientation change on the b grain boundary.     

基于访问数据模式的Cache缺失预测模型

为缓解SMT上线程对Cache的争用，提出了基于访问数据模式的Cache缺失预测模型ADM。使用模型对线程访存轨迹进行分析和计算，以两个线程在下一个时间片的访存地址信息作为模型的输入，预测Cache缺失情况并以此作为线程间Cache争用指标。 ADM实现了针对共享数据访问和私有数据访问两种模式的缺失计算方法，对比分析表明，ADM加入了对共享数据情况的分析过程，分别计算针对不同模式访存序列，结果更为精确，仿真试验表明，Cache缺失预测模型结果与目前同类模型的预测结果相比，误差分布在合理的范围内，当两个访存序列中有较多共享数据时，使用SMM方法计算结果将更为准确，证明了对访问模式进行划分的必要性。     

激励机制在大学英语教学中的运用

建立英语教学的激励机制,充分发挥学生的学习潜能,可采取创设语言环境,组织学生参加活动,利用外部动机和内部动机,激发学生对学习内容的直接兴趣等具体措施,以便使每一位学生都有同样的机会发挥自己的英语才能     

The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission

The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ～60 MeV to ～2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere.