钛合金TC4与1Cr18Ni9Ti不锈钢的扩散焊工艺探索

选有纯铜和纯镍作为中间层金属，探索ＴＣ４钛合金和１Ｃｒ８Ｎｉ９Ｔｉ不锈钢的真空扩散焊工艺，采用金相法，扫描电镜，Ｘ射线衍射等手段对接头界面附近的微区进行了较详细的分析，结果表明，采用上述中间层进行ＴＣ４－１Ｃｒ１８Ｎｉ９Ｔｉ的扩散焊时，Ｃｕ和Ｔｉ产生强烈的共晶反应，但并末阻止Ｔｉ向不锈钢中扩散，各元素相互扩散的结果，使接头中形成多层次的不同组织和多种化合物，导致接头强度较低，呈脆性断裂。     

基于XFEM-CZM耦合法的胶接接头裂纹扩展分析及强度预测

采用扩展有限元法（XFEM）和内聚力模型（CZM）相耦合的方法，分析胶接接头胶层内部裂纹扩展、界面脱粘分层现象。采用内聚力单元和内聚力接触描述胶层/板材界面，建立单/双搭接接头有限元模型。预测拉伸载荷下接头的强度性能并与已有试验数据对比分析，验证XFEM-CZM耦合法的可行性及内聚力单元和内聚力接触2种界面建模方法的有效性。模拟裂纹从胶层内部扩展至胶层/板材界面并引起界面脱粘分层的过程，分析其损伤失效机理。讨论初始裂纹长度和界面刚度、强度及应变能释放率对胶接接头强度性能的影响。结果表明:胶接接头强度随初始裂纹长度增加而降低，且在双搭接接头模型中表现更为明显；界面刚度、强度对胶接接头强度影响较大而应变能释放率的影响较小。      

复合材料单搭接胶接接头试验研究与数值模拟

针对不同搭接长度和不同被胶接件厚度的T300/QY8911层合板单搭接胶接接头进行了试验研究和数值模拟.建立了不同试验参数下的三维有限元模型,基于Hashin准则和连续介质损伤力学(CDM,Continuum Damage Mechanics)预测层合板面内损伤的起始和演化,应用黏聚区模型(CZM,Cohesive Zone Model)模拟层合板的分层损伤及胶层的失效.系统地研究了接头在不同参数下的失效模式、破坏形貌和极限载荷等的变化,模拟结果与试验吻合良好,验证了有限元分析模型的有效性.通过对接头的破坏形貌和应力分布进一步分析发现,胶接连接的失效模式和极限载荷均与胶接长度和被胶接件厚度有关;模拟接头胶接区在不同加载时刻的应力分布变化,反映了胶接连接在拉伸载荷下的破坏起始和演化过程.     

共轭梯度－快速傅里叶变换解齿状结构散射场

利用共轭梯度－快速傅里叶变换法（ＣＧ－ＦＦＴ）求解了谐振区齿状散射目标的雷达散射截面（ＲＣＳ）．通过共轭梯度－快速傅里叶变换求解电场积分方程（Ｅ－ＦＩＥ），给出齿状散射体的雷达散射截面．适当选取基函数和检验函数，将电场积分方程离散化，从而获致准确度较高的ＣＧ－ＦＦＴ实用程序，节省内存，提高了计算速度，缩短了计算时间．     

晶体振荡器的应用及发展MCXO晶振的必要性

介绍了晶体振荡器在国内外的广泛应用和ＭＣＸＯ晶振的原理方案及其较之ＴＣＸＯ晶振的各种优越性。ＭＣＸＯ晶体振荡器结合了ＳＣ切等特殊晶体的特性及微型计算机技术，对晶体振荡器和高准确度频率源的长远发展有重要意义。     

机械振动与冲击国内外标准化近况

机械振动与冲击国内外标准化近况林鸿初１引言国际标准化组织ＩＳＯ／ＴＣ１０８是负责组织起草、制订、审定和修改国际关于机械振动与冲击方面标准化文件的机构。目前，ＴＣ１０８主席是美国人Ｄ．Ｍｕｓｔｅｒ。参加国际标准化组织ＩＳＯ的成员国根据其开展活动的情况和...     

几种256Kbit SRAM芯片的单粒子翻转规律

给出了实践４号（ＳＪ－４）星载ＩＤＴ７１２５６Ｄ高速ＣＭＯＳ静态存储器和ＨＭ８８３２异步静态存储器单粒子事件（ＳＥＵ）的总翻转率,器件类型翻转率,逻辑状态翻转率,并与国外某些卫星的监测结果进行了比较。另外对部分ＳＥＵ数据进行了统计分析,给出了ＳＥＵ的片上地址和到达时间差的分布规律及拟合曲线。     

一种多目标跟踪数据处理器的设计

介绍了一种机载多目标跟踪数据处理器的实现算法．这个处理器是用专用数字信号处理芯片ＴＭＳ３２０Ｃ３０实现的，其输入的观测数据是由雷达视频回波信号经过数据采集、信号检测和目标参数提取后得到的测量数据．在实验室环境下，当信噪比为３：１时，此数据处理器在１００ｋｍ距离处的滤波估计误差为５０ｍ，方位估计误差达到半功率波束度宽的．     

从ACCV‘95看计算机视觉技术的发展

介绍了第二届亚洲计算机视觉会议（ＳＥＣＯＮＤ ＡＳＩＡＮ ＣＯＮＦＥＲ－ＥＮＣＥ ＯＮ ＣＯＭＰＵＴＥＲ ＶＩＳＩＯＮ，ＡＣＣＶ’９５）的一些情况；回顾了在该领域及相关学科的研究成果，讨论了当前计算机视觉所面临的理论与实际应用问题，并对中国空间技术研究院这一学科的发展提出看法。     

武昌地区急始型磁暴期间电离层电子总含量的变化

利用１９８０年４月至１９９０年１２月共１３６次急始型磁暴资料统计研究了武昌地区ＴＥＣ的变化。结果表明，ＴＥＣ的暴时变化出现正相，相对变化值ΔＴＥＣ的暴时变化形态与中高纬地区一些台站所观测到的结果差别较大；如果磁暴急始出现在白天，则急始后３６小时，会出现ΔＴＥＣ的极大值，如果急始出现在夜间，则不会出现极大值，这一现象与太阳黑子数，季节无关。     

Scaling analysis and model estimation of solar corona index

A monthly average solar green coronal index time series for the period from January 1939 to December 2008 collected from NOAA (The National Oceanic and Atmospheric Administration) has been analysed in this paper in perspective of scaling analysis and modelling. Smoothed and de-noising have been done using suitable mother wavelet as a pre-requisite. The Finite Variance Scaling Method (FVSM), Higuchi method, rescaled range (R/S) and a generalized method have been applied to calculate the scaling exponents and fractal dimensions of the time series. Autocorrelation function (ACF) is used to find autoregressive (AR) process and Partial autocorrelation function (PACF) has been used to get the order of AR model. Finally a best fit model has been proposed using Yule-Walker Method with supporting results of goodness of fit and wavelet spectrum. The results reveal an anti-persistent, Short Range Dependent (SRD), self-similar property with signatures of non-causality, non-stationarity and nonlinearity in the data series. The model shows the best fit to the data under observation.     

Stochastic particle acceleration by the forced interaction of relativistic current sheets

We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ^−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles.     

Development of a gas chromatography compatible Sample Processing System (SPS) for the in-situ analysis of refractory organic matter in martian soil: preliminary results

In the frame of the 2009 Mars Science Laboratory (MSL) mission a new sample preparation system (SPS) compatible with gas chromatography–mass spectrometry (GC–MS) has been developed for the in situ analysis of complex organic molecules in the Martian soil. The goal is to detect, if they exist, some of the key compounds that play an important role in life on Earth including carboxylic acids, amino acids and nucleobases.     

基于LuGre模型的电液加载系统摩擦补偿

为了提高电液加载系统控制精度,针对摩擦问题提出了基于LuGre摩擦模型的前馈补偿方法.建立了用于摩擦仿真分析和补偿器设计的电液加载系统数学模型;通过实验获取并分析了相关的摩擦数据;基于实验数据进行LuGre模型参数辨识,把LuGre模型和辨识结果引入电液加载系统数学模型,并进行仿真结果与实际摩擦数据的对照,证明了LuGre摩擦模型的准确性.设计前馈补偿器,进行了实验对比,实验结果表明前馈补偿器可将摩擦产生的控制误差有效地降至未补偿时的30%左右.      

Concept options for the aerial survey of Titan

Various aerial platforms intended for long endurance survey of the Titan surface are presented. A few novel concepts are introduced, including a heated methane balloon and a balloon with a tethered wind turbine. All the concept options are predicted to have lower scientific payload fractions than the Huygens probe. It is concluded that the selection of the best aerial platform option depends on more accurate mass estimates and a clear decision on whether, or not, in situ surface composition measurements are required in conjunction with aerial remote sensing.     

Heterogeneous solid/gas chemistry of organic compounds related to comets,meteorites, Titan,and Mars: Laboratory and in lower Earth orbit experiments

To understand the evolution of organic molecules involved in extraterrestrial environments and with exobiological implications, many experimental programs in the laboratory are devoted to photochemical studies in the gaseous phase as well as in the solid state. The validity of such studies and their applications to extraterrestrial environments can be questioned as long as experiments conducted in space conditions, with the full solar spectrum, especially in the short wavelength domain, have not been implemented. The experiments that are described here will be carried out on a FOTON capsule, using the BIOPAN facility, and on the International Space Station, using the EXPOSE facility. Vented and sealed exposition cells will be used, which will allow us to study the chemical evolution in the gaseous phase as well as heterogeneous processes, such as the degradation of solid compounds and the release of gaseous fragments.     

CoRoT and Kepler results: Solar-like oscillators

The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars. These data have revolutionized the fields of transiting exoplanets and asteroseismology. In this review some important asteroseismic results obtained using data from the CoRoT and Kepler space missions concerning stars that show solar-like oscillations are discussed. These results comprise, among others, measurements of the location of the base of the convection zone and helium second-ionization zone in main-sequence stars, the presence (or not) of core-helium burning in red-giant stars, as well as differential rotation in these stars.     

Return to Europa: Overview of the Jupiter Europa orbiter mission

Missions to explore Europa have been imagined ever since the Voyager mission first suggested that Europa was geologically very young. Subsequently, the Galileo spacecraft supplied fascinating new insights into this satellite of Jupiter. Now, an international team is proposing a return to the Jupiter system and Europa with the Europa Jupiter System Mission (EJSM). Currently, NASA and ESA are designing two orbiters that would explore the Jovian system and then each would settle into orbit around one of Jupiter’s icy satellites, Europa and Ganymede. In addition, the Japanese Aerospace eXploration Agency (JAXA) is considering a Jupiter magnetospheric orbiter and the Russian Space Agency is investigating a Europa lander.     

HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

Radioactivity of the Moon and planets

In this report the main results of the study of radioactivity of the solar sistem bodies are considered. The radioactivity of the Moon and planets was measured by means of vehicles in situ. The radioactivity of the lunar samples, brought to the Earth was studied with laboratory equipment.