基于结构件实例库的飞机机体结构快速建模

为充分利用和借鉴已有的飞机结构件设计方案实例信息,研究了面向对象的参数化结构件实例描述方法,提出了飞机结构件实例库的总体框架并开发了系统的原型.研究了基于实例库的飞机机体结构设计措施及建模方法,提出了翼面结构和机身结构的参数化描述和模型构建方法,并在一个开放式的飞机总体设计环境中完成了基于实例库的飞机结构快速设计功能.最后通过应用示例说明了该系统和方法的有效性.     

二维有限元网格全自动生成

利用ＰＥＤＳ（ＰａｒａｍｅｔｒｉｃＥｎｇｉｎｅｅｒｉｎｇＤｅｓｉｇｎＳｙｓｅｍ）造型系统的几何，拓扑信息实现了二维有限元网格自动生成，在实现过程中，改进了Ｗａｓｔｏｎ三角化算法，把此方法应用到有限元剖分中，还利用了迭代的Ｌａｐｌａｃｉａｎ算法对网格进行了均匀化处理，另外，还提供了可靠，快速对网格编辑，局部细化的方法，最终使有限元网格生成完全自动化，而且速度快，质量好，密度易于控制。     

离散事件动态系统的GSMP模型及扰动分析

对离散事件动态系统（ＤＥＤＳ）的仿真过程建立了包含中断事件集和驱动事件集的广义半马尔可夫过程（ＧＳＭＰ）模型，对参数的无穷小扰动所引起的系统状态转移时刻进行了扰动分析，最后，讨论了扰动分析所需要的可变换条件和样本性能函数的关系，并提出值得进一步研究的问题。     

基于组装的过程工程环境

描述了一个基于组装的过程工程环境，该环境包括过程定义，过程实例化，过程模拟，过程动作４个部分，采用了基于组装的过程建模方法，能够对重用过程库中的过程部件进行组装，生成新的过程模型，并由过程模型驱动实际运作。     

三维表面微观形貌的表征参数和方法

近几年,由于计算能力、速度和图像、数据处理技术的不断提高,极大地推进了３Ｄ表面微观形貌测量仪的实用化和商品化,同时也增加了研究者对３Ｄ分析的兴趣。总结了近期文献中出现的３Ｄ分析方法和表征参数,如：基准表面、图形（ 像） 表征、参数表征以及Ｍｏｔｉｆ 和分形表征方法,旨在促进我国对３Ｄ表面研究的发展。最后提出了３Ｄ表征技术的任务和发展方向。     

三维重建的飞机机动动作库设计与可视化

机动动作库是飞机空战仿真的重要基础,可靠的、具有针对性的机动动作库能够提高空战仿真的真实性和应用价值。为了建立具有针对性的机动动作库,提出了一种通过三维逆向建模进行气动特性计算再建立飞机机动动作库的技术途径,对气动参数未知飞机的空战仿真问题提供了技术支撑。首先,对飞机的几何外形进行了三维重建,计算分析了其纵向气动特性;然后,将气动数据加入飞行仿真的限制环节,设计了针对该型飞机典型战术动作的机动动作库;最后,基于MATLAB函数进行了机动动作的可视化研究。研究结果表明:机动动作库体现了对于飞机类型的针对性和可靠性,可视化实现了飞行轨迹和飞机姿态的三维显示及参数游标,为空战决策、空战仿真模拟训练和提高作战效能奠定了基础。      

基于特征造型技术的涡轮叶片参数化设计

针对航空发动机涡轮气冷叶片的结构特点,提出了叶片参数化建模的特征分类形式.然后,利用特征造型技术开发涡轮叶片的参数化设计系统;并以直背涡轮叶片为具体实例阐述了该参数化模块的开发过程,为航空发动机典型结构件的参数化奠定了基础.      

可渗透各向同性多孔材料动静压轴承性能研究

利用Ｒｅｙｎｏｌｄｓ和Ｌａｐｌａｃｅ方程以及Ｄａｒｃｙ定律，导出了可渗透各向同性材料动静压窄轴承的计算方程．计算结果显示出这种轴承具有承载力高和姿态角小的特点，并指出设计参数之间存在优化组合．     

可渗秀各向同性多孔材料动静压轴承性能研究

利用Ｒｅｙｎｏｌｄｓ和Ｌａｐｌａｃｅ方程以及Ｄａｒｃｙ定律，导出了可渗透各向同性动静压窄轴承的计算方程。计算结果显示出这种轴承具有承载力高和姿态角小的特点，并指出设计参数之间存在优化组合。     

对技术引进和经济规模有效性的分析

采用数据包络分析法（ＤａｔａＥｎｖｅｌｏｐｍｅｎｔＡｎａｌｙｓｉｓ，ＤＥＡ法）对技术引进有效性及经济规模有效进行评价，其参数选择原则为绝对数系列，以轴承行业５０家企业的数据，对同一时间点的现有生产配置条件下的企业经济规模有效性进行横向评价，以某厂８年数据对不同时间点企业技术引进的后期效果进行技术引进有效性纵向评价。     

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.     

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.     

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.      

The ESA scientific programme

The ESA scientific programme has, so far, provided several significant astrophysics experiments and further important missions are scheduled for execution during the next decade. These missions are briefly summarised together with several astrophysics investigations presently under study.     

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.